SweConst

java.lang.Object
- swisseph.SweConst

All Implemented Interfaces:

java.io.Serializable
```
public class SweConst
extends java.lang.Object
implements java.io.Serializable
```
This class contains all the constants that might be interesting to the user of the swisseph package.
All constants are static, so there is no need to instantiate the class.
You will find the complete documentation for the original SwissEphemeris package at http://www.astro.ch/swisseph/sweph_g.htm. By far most of the information there is directly valid for this port to Java as well.

See Also:

Serialized Form

Field Summary

Fields
Modifier and Type	Field and Description
`static double`	`AUNIT`
`static int`	`ERR` Constant for unsuccessful return values.
`static int`	`OK` Constant for successful return values.
`static int`	`SE_ACRONYCHAL_RISING`
`static int`	`SE_ACRONYCHAL_SETTING`
`static int`	`SE_ADMETOS` The number of the Hamburger or Uranian "planet" admetos.
`static int`	`SE_APOLLON` The number of the Hamburger or Uranian "planet" appollon.
`static int`	`SE_APP_TO_TRUE` Calculate the true altitude from the apparent altitude.
`static int`	`SE_ARMC` This is a constant to access the value of the sidereal time in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the sidereal time as an object in transit calculations.
`static int`	`SE_ASC` This is a constant to access the ascendant value in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the ascendant object in transit calculations.
`static int`	`SE_AST_OFFSET` The offset, where asteroid numbers start.
`static int`	`SE_BIT_ASTRO_TWILIGHT`
`static int`	`SE_BIT_CIVIL_TWILIGHT`
`static int`	`SE_BIT_DISC_BOTTOM` Add this to SE_CALC_RISE/SET, if rise or set of disc bottom is requested.
`static int`	`SE_BIT_DISC_CENTER` Add this to SE_CALC_RISE/SET, if rise or set of disc center is requested.
`static int`	`SE_BIT_FIXED_DISC_SIZE`
`static int`	`SE_BIT_NAUTIC_TWILIGHT`
`static int`	`SE_BIT_NO_REFRACTION` Add this to SE_CALC_RISE/SET, if refraction should not to be considered.
`static int`	`SE_CALC_ITRANSIT` Calculate the time of the lower meridian transit (northern, below the horizon).
`static int`	`SE_CALC_MTRANSIT` Calculate the time of the upper meridian transit (southern for northern geo.
`static int`	`SE_CALC_RISE` Calculate the time of sunrise.
`static int`	`SE_CALC_SET` Calculate the time of sunset.
`static int`	`SE_CERES` planet number of ceres.
`static int`	`SE_CHIRON` planet number of chiron.
`static int`	`SE_COASC1` This is a constant to access the value of the "co-ascendant" of W.
`static int`	`SE_COASC2` This is a constant to access the value of the "co-ascendant" of M.
`static int`	`SE_COSMICAL_SETTING`
`static int`	`SE_CUPIDO` The number of the Hamburger or Uranian "planet" cupido.
`static int`	`SE_DE_NUMBER`
`static int`	`SE_EARTH` planet number of the earth.
`static int`	`SE_ECL_1ST_VISIBLE` Begin of partial eclipse.
`static int`	`SE_ECL_2ND_VISIBLE` Begin of total eclipse.
`static int`	`SE_ECL_3RD_VISIBLE` End of total eclipse.
`static int`	`SE_ECL_4TH_VISIBLE` End of partial eclipse.
`static int`	`SE_ECL_ALLTYPES_LUNAR`
`static int`	`SE_ECL_ALLTYPES_SOLAR`
`static int`	`SE_ECL_ANNULAR` Annular eclipse.
`static int`	`SE_ECL_ANNULAR_TOTAL`
`static int`	`SE_ECL_CENTRAL`
`static int`	`SE_ECL_MAX_VISIBLE`
`static int`	`SE_ECL_NONCENTRAL`
`static int`	`SE_ECL_NUT` Planet number for the ipl parameter in swe_calc*().
`static int`	`SE_ECL_OCC_BEG_DAYLIGHT` Occultation begins during the day
`static int`	`SE_ECL_OCC_END_DAYLIGHT` Occultation ends during the day
`static int`	`SE_ECL_ONE_TRY` Just check if the next conjunction of the moon with a planet is an occultation; don't search further.
`static int`	`SE_ECL_PARTBEG_VISIBLE` Begin of partial eclipse.
`static int`	`SE_ECL_PARTEND_VISIBLE` End of partial eclipse.
`static int`	`SE_ECL_PARTIAL`
`static int`	`SE_ECL_PENUMBBEG_VISIBLE` Begin of penumbral eclipse.
`static int`	`SE_ECL_PENUMBEND_VISIBLE` End of penumbral eclipse.
`static int`	`SE_ECL_PENUMBRAL`
`static int`	`SE_ECL_TOTAL`
`static int`	`SE_ECL_TOTBEG_VISIBLE` Begin of total eclipse.
`static int`	`SE_ECL_TOTEND_VISIBLE` End of total eclipse.
`static int`	`SE_ECL_VISIBLE`
`static int`	`SE_ECL2HOR` This is a constant to be used as a flag to swe_azalt().
`static java.lang.String`	`SE_EPHE_PATH` Ephemeris path.
`static int`	`SE_EQU2HOR` This is a constant to be used as a flag to swe_azalt().
`static int`	`SE_EQUASC` This is a constant to access the value of the "equatorial ascendant" in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the equatorial ascendant object in transit calculations.
`static int`	`SE_EVENING_FIRST`
`static int`	`SE_EVENING_LAST`
`static int`	`SE_FICT_OFFSET_1`
`static int`	`SE_FIXSTAR`
`static java.lang.String`	`SE_FNAME_DE200`
`static java.lang.String`	`SE_FNAME_DE403`
`static java.lang.String`	`SE_FNAME_DE404`
`static java.lang.String`	`SE_FNAME_DE405`
`static java.lang.String`	`SE_FNAME_DE406`
`static java.lang.String`	`SE_FNAME_DE431`
`static java.lang.String`	`SE_FNAME_DFT`
`static java.lang.String`	`SE_FNAME_DFT2`
`static int`	`SE_HADES` The number of the Hamburger or Uranian "planet" hades.
`static int`	`SE_HARRINGTON` The "planet" number of the fictitious body harrington.
`static int`	`SE_HELFLAG_AV`
`static int`	`SE_HELFLAG_AVKIND`
`static int`	`SE_HELFLAG_AVKIND_MIN7`
`static int`	`SE_HELFLAG_AVKIND_MIN9`
`static int`	`SE_HELFLAG_AVKIND_PTO`
`static int`	`SE_HELFLAG_AVKIND_VR`
`static int`	`SE_HELFLAG_HIGH_PRECISION`
`static int`	`SE_HELFLAG_LONG_SEARCH`
`static int`	`SE_HELFLAG_NO_DETAILS`
`static int`	`SE_HELFLAG_OPTICAL_PARAMS`
`static int`	`SE_HELFLAG_SEARCH_1_PERIOD`
`static int`	`SE_HELFLAG_VISLIM_DARK`
`static int`	`SE_HELFLAG_VISLIM_NOMOON`
`static int`	`SE_HELFLAG_VISLIM_PHOTOPIC`
`static int`	`SE_HELIACAL_AVKIND`
`static int`	`SE_HELIACAL_AVKIND_MIN7`
`static int`	`SE_HELIACAL_AVKIND_MIN9`
`static int`	`SE_HELIACAL_AVKIND_PTO`
`static int`	`SE_HELIACAL_AVKIND_VR`
`static int`	`SE_HELIACAL_HIGH_PRECISION`
`static int`	`SE_HELIACAL_LONG_SEARCH`
`static int`	`SE_HELIACAL_NO_DETAILS`
`static int`	`SE_HELIACAL_OPTICAL_PARAMS`
`static int`	`SE_HELIACAL_RISING`
`static int`	`SE_HELIACAL_SEARCH_1_PERIOD`
`static int`	`SE_HELIACAL_SETTING`
`static int`	`SE_HELIACAL_VISLIM_DARK`
`static int`	`SE_HELIACAL_VISLIM_NOMOON`
`static int`	`SE_HELIACAL_VISLIM_PHOTOPIC`
`static int`	`SE_HOR2ECL` This is a constant to be used as a flag to swe_azalt_rev().
`static int`	`SE_HOR2EQU` This is a constant to be used as a flag to swe_azalt_rev().
`static int`	`SE_HOUSE1`
`static int`	`SE_HOUSE10`
`static int`	`SE_HOUSE11`
`static int`	`SE_HOUSE12`
`static int`	`SE_HOUSE2`
`static int`	`SE_HOUSE3`
`static int`	`SE_HOUSE4`
`static int`	`SE_HOUSE5`
`static int`	`SE_HOUSE6`
`static int`	`SE_HOUSE7`
`static int`	`SE_HOUSE8`
`static int`	`SE_HOUSE9`
`static int`	`SE_HSYS_ALCABITIUS`
`static int`	`SE_HSYS_CAMPANUS`
`static int`	`SE_HSYS_EQUAL`
`static int`	`SE_HSYS_GAUQUELIN_SECTORS`
`static int`	`SE_HSYS_HORIZONTAL`
`static int`	`SE_HSYS_KOCH`
`static int`	`SE_HSYS_KRUSINSKI`
`static int`	`SE_HSYS_MERIDIAN`
`static int`	`SE_HSYS_MORINUS`
`static int`	`SE_HSYS_PLACIDUS`
`static int`	`SE_HSYS_POLICH_PAGE`
`static int`	`SE_HSYS_PORPHYRIUS`
`static int`	`SE_HSYS_REGIOMONTANUS`
`static int`	`SE_HSYS_VEHLOW`
`static int`	`SE_HSYS_WHOLE_SIGN`
`static int`	`SE_INTP_APOG` planet number of the interpolated lunar agopee.
`static int`	`SE_INTP_PERG` planet number of the interpolated lunar perigee.
`static int`	`SE_ISIS` The "planet" number of the fictitious body isis.
`static int`	`SE_JUNO` planet number of juno.
`static int`	`SE_JUPITER` planet number of jupiter.
`static int`	`SE_KRONOS` The number of the Hamburger or Uranian "planet" kronos.
`static int`	`SE_MARS` planet number of mars.
`static int`	`SE_MC` This is a constant to access the medium coeli value in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the medium coeli object in transit calculations.
`static int`	`SE_MEAN_APOG` (planet) number of the mean apogee (== Lilith).
`static int`	`SE_MEAN_NODE` (planet) number of the mean moon node.
`static int`	`SE_MERCURY` planet number of mercury.
`static int`	`SE_MIXEDOPIC_FLAG`
`static int`	`SE_MODEL_BIAS`
`static int`	`SE_MODEL_DELTAT`
`static int`	`SE_MODEL_JPLHOR_MODE`
`static int`	`SE_MODEL_JPLHORA_MODE`
`static int`	`SE_MODEL_NUT`
`static int`	`SE_MODEL_PREC_LONGTERM`
`static int`	`SE_MODEL_PREC_SHORTTERM`
`static int`	`SE_MODEL_SIDT`
`static int`	`SE_MOON` planet number of the moon.
`static int`	`SE_MORNING_FIRST`
`static int`	`SE_MORNING_LAST`
`static int`	`SE_NASCMC` This is a constant to know the count of valid parameters in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses().
`static int`	`SE_NEPTUNE` planet number of neptune.
`static int`	`SE_NEPTUNE_ADAMS` The "planet" number of the fictitious body neptune-adams.
`static int`	`SE_NEPTUNE_LEVERRIER` The "planet" number of the fictitious body neptune-leverrier.
`static int`	`SE_NIBIRU` The "planet" number of the fictitious body nibiru.
`static int`	`SE_NODBIT_FOPOINT` Used for swe_nod_aps(): focal point of orbit instead of aphelion
`static int`	`SE_NODBIT_MEAN` Used for swe_nod_aps(): mean nodes/apsides
`static int`	`SE_NODBIT_OSCU` Used for swe_nod_aps(): osculating nodes/apsides
`static int`	`SE_NODBIT_OSCU_BAR` Used for swe_nod_aps(): osculating nodes/apsides, but motion about solar system barycenter is considered
`static int`	`SE_OSCU_APOG` (planet) number of the osculating apogee.
`static int`	`SE_PALLAS` planet number of pallas.
`static int`	`SE_PHOLUS` planet number of pholus.
`static int`	`SE_PHOTOPIC_FLAG`
`static int`	`SE_PLUTO` planet number of pluto.
`static int`	`SE_PLUTO_LOWELL` The "planet" number of the fictitious body pluto-lowell.
`static int`	`SE_PLUTO_PICKERING` The "planet" number of the fictitious body pluto-pickering.
`static int`	`SE_POLASC` This is a constant to access the polar ascendant value of M.
`static int`	`SE_POSEIDON` The number of the Hamburger or Uranian "planet" poseidon.
`static int`	`SE_PROSERPINA` The "planet" number of the fictitious body "Proserpina".
`static int`	`SE_SATURN` planet number of saturn.
`static int`	`SE_SCOTOPIC_FLAG`
`static int`	`SE_SIDBIT_ECL_T0` This specifies that sidereal calculations are done via a projection onto the ecliptic at date t0.
`static int`	`SE_SIDBIT_SSY_PLANE` This specifies that sidereal calculations are done via a projection onto the solar system plane.
`static int`	`SE_SIDBITS`
`static int`	`SE_SIDM_ALDEBARAN_15TAU` A constant to be used for specifying the sidereal mode (ayanamsha) as defining t0 by Aldebaran at 15 degrees Taurus.
`static int`	`SE_SIDM_ARYABHATA` A constant to be used for specifying the sidereal mode (ayanamsha) as ARYABHATA (Aryabhata, same date as SE_SIDM_SURYASIDDHANTA_MSUN, but UT 6:56:55.57).
`static int`	`SE_SIDM_ARYABHATA_MSUN` A constant to be used for specifying the sidereal mode (ayanamsha) as ARYABHATA_MSUN (Aryabhata, analogous SE_SIDM_SURYASIDDHANTA_MSUN).
`static int`	`SE_SIDM_B1950` A constant to be used for specifying the sidereal mode (ayanamsha) as B1950 (Julian day 2433282.42345905, 1950 January 0.923).
`static int`	`SE_SIDM_BABYL_ETPSC` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Mercier.
`static int`	`SE_SIDM_BABYL_HUBER` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Huber.
`static int`	`SE_SIDM_BABYL_KUGLER1` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Kugler 1.
`static int`	`SE_SIDM_BABYL_KUGLER2` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Kugler 2.
`static int`	`SE_SIDM_BABYL_KUGLER3` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Kugler 3.
`static int`	`SE_SIDM_DELUCE` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by De Luce.
`static int`	`SE_SIDM_DJWHAL_KHUL` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Djwhal Khool.
`static int`	`SE_SIDM_FAGAN_BRADLEY` A constant to be used for specifying the sidereal mode (ayanamsha).
`static int`	`SE_SIDM_GALCENT_0SAG` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by the galactic center being at 0 degrees Sagittarius.
`static int`	`SE_SIDM_HIPPARCHOS` A constant to be used for specifying the sidereal mode (ayanamsha) by defined by Hipparchos.
`static int`	`SE_SIDM_J1900` A constant to be used for specifying the sidereal mode (ayanamsha) as J1900 (Julian day 2415020.0, 1900 January 0.5).
`static int`	`SE_SIDM_J2000` A constant to be used for specifying the sidereal mode (ayanamsha) as J2000 (Julian day 2451545.0, 2000 January 1.5)
`static int`	`SE_SIDM_JN_BHASIN` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by JN Bhasin.
`static int`	`SE_SIDM_KRISHNAMURTI` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Krishnamurti.
`static int`	`SE_SIDM_LAHIRI` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Lahiri.
`static int`	`SE_SIDM_RAMAN` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Raman.
`static int`	`SE_SIDM_SASSANIAN` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Sassanian.
`static int`	`SE_SIDM_SS_CITRA` A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_SS_CITRA (SS, Citra/Spica at polar long. 180°).
`static int`	`SE_SIDM_SS_REVATI` A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_SS_REVATI (SS, Revati/zePsc at polar long. 359°50').
`static int`	`SE_SIDM_SURYASIDDHANTA` A constant to be used for specifying the sidereal mode (ayanamsha) as SURYASIDDHANTA (Suryasiddhanta, assuming ingress of mean Sun into Aries at point of mean equinox of date on 21.3.499, noon, Ujjain (75.7684565 E) = 7:30:31.57 UT).
`static int`	`SE_SIDM_SURYASIDDHANTA_MSUN` A constant to be used for specifying the sidereal mode (ayanamsha) as SURYASIDDHANTA_MSUN (Suryasiddhanta, assuming ingress of mean Sun into Aries at true position of mean Sun at same epoch).
`static int`	`SE_SIDM_TRUE_CITRA` A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_TRUE_CITRA (True Spica (Spica exactly at 0 Libra)
`static int`	`SE_SIDM_TRUE_PUSHYA` A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_TRUE_PUSHYA (True Pushya (delta Cnc exactly a 16 Cancer))
`static int`	`SE_SIDM_TRUE_REVATI` A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_TRUE_REVATI (True Revati (zeta Psc exactly at 0 Aries))
`static int`	`SE_SIDM_USER` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by the user in the additional two parameters of swe_set_sid_mode().
`static int`	`SE_SIDM_USHASHASHI` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Ushashashi.
`static int`	`SE_SIDM_YUKTESHWAR` A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Sri Yukteshwar.
`static int`	`SE_SPLIT_DEG_KEEP_DEG` SwissLib.swe_split_deg(): Don't round to next degree, e.g. 13.9999999 will be rounded to 13d59'59" (or 13d59' or 13d)
`static int`	`SE_SPLIT_DEG_KEEP_SIGN` SwissLib.swe_split_deg(): Don't round to next sign, e.g. 29.9999999 will be rounded to 29d59'59" (or 29d59' or 29d)
`static int`	`SE_SPLIT_DEG_ROUND_DEG`
`static int`	`SE_SPLIT_DEG_ROUND_MIN`
`static int`	`SE_SPLIT_DEG_ROUND_SEC`
`static int`	`SE_SPLIT_DEG_ZODIACAL`
`static int`	`SE_SUN` planet number of the sun.
`static double`	`SE_TIDAL_26`
`static double`	`SE_TIDAL_AUTOMATIC`
`static double`	`SE_TIDAL_DE200`
`static double`	`SE_TIDAL_DE403`
`static double`	`SE_TIDAL_DE404`
`static double`	`SE_TIDAL_DE405`
`static double`	`SE_TIDAL_DE406`
`static double`	`SE_TIDAL_DE421`
`static double`	`SE_TIDAL_DE430`
`static double`	`SE_TIDAL_DE431`
`static double`	`SE_TIDAL_DEFAULT`
`static double`	`SE_TIDAL_JPLEPH`
`static double`	`SE_TIDAL_MOSEPH`
`static double`	`SE_TIDAL_SWIEPH`
`static int`	`SE_TRUE_NODE` (planet) number of the true moon node.
`static int`	`SE_TRUE_TO_APP` Calculate the apparent altitude from the true altitude.
`static int`	`SE_URANUS` planet number of uranus.
`static int`	`SE_VARUNA`
`static int`	`SE_VENUS` planet number of venus.
`static int`	`SE_VERTEX` This is a constant to access the vertex value in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the vertex object in transit calculations.
`static int`	`SE_VESTA` planet number of vesta.
`static int`	`SE_VULCAN` The "planet" number of the fictitious body vulcan.
`static int`	`SE_VULKANUS` The number of the Hamburger or Uranian "planet" vulkanus.
`static int`	`SE_WALDEMATH` The "planet" number of the fictitious body "Waldemath".
`static int`	`SE_WHITE_MOON` The "planet" number of the fictitious body "white moon" (== Selena).
`static int`	`SE_ZEUS` The number of the Hamburger or Uranian "planet" zeus.
`static int`	`SEFLG_BARYCTR` Calculate barycentric positions.
`static int`	`SEFLG_DEFAULTEPH` Defines the default method of calculation as SEFLG_SWIEPH.
`static int`	`SEFLG_DPSIDEPS_1980`
`static int`	`SEFLG_EPHMASK`
`static int`	`SEFLG_EQUATORIAL` Calculate the position of the planet in the earth equator coordinate system.
`static int`	`SEFLG_HELCTR` Calculate the heliocentric position of the planet.
`static int`	`SEFLG_ICRS` Calculate in the "International Celestial Reference System."
`static int`	`SEFLG_J2000` Calculate the position of the planet without considering the precession, i.e., calculate J2000 equinox.
`static int`	`SEFLG_JPLEPH` Use the calculation routines that use the ephemeris data files of the Solar System Dynamics Group of the Jet Propulsion Laboratory of NASA http://ssd.jpl.nasa.gov/.
`static int`	`SEFLG_JPLHOR`
`static int`	`SEFLG_JPLHOR_APPROX`
`static int`	`SEFLG_MOSEPH` Use the Moshier semi-analytical calculation routines.
`static int`	`SEFLG_NOABERR` Calculate the position of the planet without considering the 'annual' aberration of light.
`static int`	`SEFLG_NOGDEFL` Calculate the position of the planet without considering gravitational deflection.
`static int`	`SEFLG_NONUT` Calculate the position of the planet without considering the nutation, i.e., calculate the mean equinox of the day.
`static int`	`SEFLG_PARTILE_TRANSIT` calculate partile transits.
`static int`	`SEFLG_PARTILE_TRANSIT_END` calculate partile transits.
`static int`	`SEFLG_PARTILE_TRANSIT_START` calculate partile transits.
`static int`	`SEFLG_RADIANS` Return coordinates in radians instead of degrees.
`static int`	`SEFLG_SIDEREAL` Calculate sidereal positions.
`static int`	`SEFLG_SPEED` Calculate the speed of the planet.
`static int`	`SEFLG_SPEED3` Calculate the speed of the planet.
`static int`	`SEFLG_SWIEPH` Use the calculation routines of Swiss Ephemeris from Astrodienst AG Zürich http://www.astro.com.
`static int`	`SEFLG_TOPOCTR` Calculate topocentric positions.
`static int`	`SEFLG_TRANSIT_DISTANCE` calculate transits over a distance in AU.
`static int`	`SEFLG_TRANSIT_LATITUDE` calculate transits over a latitude.
`static int`	`SEFLG_TRANSIT_LONGITUDE` calculate transits over a longitude.
`static int`	`SEFLG_TRANSIT_SPEED` calculate transits over a (longitudinal, latitudinal or distance) speed value.
`static int`	`SEFLG_TRUEPOS` Calculate the true position of the planet versus the apparent position.
`static int`	`SEFLG_XYZ` Return cartesian coordinates instead of polar coordinates.
`static int`	`SEFLG_YOGA_TRANSIT` calculate yoga transits, this means consider the SUM of two planets positions or speeds instead of the difference.
`static int`	`SEMOD_BIAS_DEFAULT`
`static int`	`SEMOD_BIAS_IAU2000`
`static int`	`SEMOD_BIAS_IAU2006`
`static int`	`SEMOD_DELTAT_DEFAULT`
`static int`	`SEMOD_DELTAT_ESPENAK_MEEUS_2006`
`static int`	`SEMOD_DELTAT_STEPHENSON_MORRISON_2004`
`static int`	`SEMOD_JPLHOR_DEFAULT`
`static int`	`SEMOD_JPLHOR_EXTENDED_1800`
`static int`	`SEMOD_JPLHOR_NOT_EXTENDED`
`static int`	`SEMOD_JPLHORA_1`
`static int`	`SEMOD_JPLHORA_2`
`static int`	`SEMOD_JPLHORA_DEFAULT`
`static int`	`SEMOD_NUT_DEFAULT`
`static int`	`SEMOD_NUT_IAU_1980`
`static int`	`SEMOD_NUT_IAU_2000A`
`static int`	`SEMOD_NUT_IAU_2000B`
`static int`	`SEMOD_NUT_IAU_CORR_1987`
`static int`	`SEMOD_PREC_BRETAGNON_2003`
`static int`	`SEMOD_PREC_DEFAULT`
`static int`	`SEMOD_PREC_DEFAULT_SHORT`
`static int`	`SEMOD_PREC_IAU_1976`
`static int`	`SEMOD_PREC_IAU_2000`
`static int`	`SEMOD_PREC_IAU_2006`
`static int`	`SEMOD_PREC_LASKAR_1986`
`static int`	`SEMOD_PREC_SIMON_1994`
`static int`	`SEMOD_PREC_VONDRAK_2011`
`static int`	`SEMOD_PREC_WILLIAMS_1994`
`static int`	`SEMOD_SIDT_DEFAULT`
`static int`	`SEMOD_SIDT_IERS_CONV_2010`
`static int`	`SEMOD_SIDT_LONGTERM`
`static int`	`SEMOD_SIDT_PREC_MODEL`
`static double`	`TJD_INVALID`

Method Summary
- Methods inherited from class java.lang.Object
  clone, equals, finalize, getClass, hashCode, notify, notifyAll, toString, wait, wait, wait

- Field Detail
  - OK
```
public static final int OK
```
    Constant for successful return values. It is equal to 0.
    
    See Also:
    
    Constant Field Values
  - ERR
```
public static final int ERR
```
    Constant for unsuccessful return values. It is equal to -1.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_NUT
```
public static final int SE_ECL_NUT
```
    Planet number for the ipl parameter in swe_calc*(). It does not calculate a real planet, but the ecliptic and nutation of that date. Its value is -1.
    
    See Also:
    
    Constant Field Values
  - SE_SUN
```
public static final int SE_SUN
```
    planet number of the sun. It is equal to 0.
    
    See Also:
    
    Constant Field Values
  - SE_MOON
```
public static final int SE_MOON
```
    planet number of the moon. It is equal to 1.
    
    See Also:
    
    Constant Field Values
  - SE_MERCURY
```
public static final int SE_MERCURY
```
    planet number of mercury. It is equal to 2.
    
    See Also:
    
    Constant Field Values
  - SE_VENUS
```
public static final int SE_VENUS
```
    planet number of venus. It is equal to 3.
    
    See Also:
    
    Constant Field Values
  - SE_MARS
```
public static final int SE_MARS
```
    planet number of mars. It is equal to 4.
    
    See Also:
    
    Constant Field Values
  - SE_JUPITER
```
public static final int SE_JUPITER
```
    planet number of jupiter. It is equal to 5.
    
    See Also:
    
    Constant Field Values
  - SE_SATURN
```
public static final int SE_SATURN
```
    planet number of saturn. It is equal to 6.
    
    See Also:
    
    Constant Field Values
  - SE_URANUS
```
public static final int SE_URANUS
```
    planet number of uranus. It is equal to 7.
    
    See Also:
    
    Constant Field Values
  - SE_NEPTUNE
```
public static final int SE_NEPTUNE
```
    planet number of neptune. It is equal to 8.
    
    See Also:
    
    Constant Field Values
  - SE_PLUTO
```
public static final int SE_PLUTO
```
    planet number of pluto. It is equal to 9.
    
    See Also:
    
    Constant Field Values
  - SE_MEAN_NODE
```
public static final int SE_MEAN_NODE
```
    (planet) number of the mean moon node. It is equal to 10.
    
    See Also:
    
    Constant Field Values
  - SE_TRUE_NODE
```
public static final int SE_TRUE_NODE
```
    (planet) number of the true moon node. It is equal to 11.
    
    See Also:
    
    Constant Field Values
  - SE_MEAN_APOG
```
public static final int SE_MEAN_APOG
```
    (planet) number of the mean apogee (== Lilith). It is equal to 12.
    
    See Also:
    
    Constant Field Values
  - SE_OSCU_APOG
```
public static final int SE_OSCU_APOG
```
    (planet) number of the osculating apogee. It is equal to 13.
    
    See Also:
    
    Constant Field Values
  - SE_EARTH
```
public static final int SE_EARTH
```
    planet number of the earth. It is equal to 14.
    
    See Also:
    
    Constant Field Values
  - SE_CHIRON
```
public static final int SE_CHIRON
```
    planet number of chiron. It is equal to 15.
    
    See Also:
    
    Constant Field Values
  - SE_PHOLUS
```
public static final int SE_PHOLUS
```
    planet number of pholus. It is equal to 16.
    
    See Also:
    
    Constant Field Values
  - SE_CERES
```
public static final int SE_CERES
```
    planet number of ceres. It is equal to 17.
    
    See Also:
    
    Constant Field Values
  - SE_PALLAS
```
public static final int SE_PALLAS
```
    planet number of pallas. It is equal to 18.
    
    See Also:
    
    Constant Field Values
  - SE_JUNO
```
public static final int SE_JUNO
```
    planet number of juno. It is equal to 19.
    
    See Also:
    
    Constant Field Values
  - SE_VESTA
```
public static final int SE_VESTA
```
    planet number of vesta. It is equal to 20.
    
    See Also:
    
    Constant Field Values
  - SE_INTP_APOG
```
public static final int SE_INTP_APOG
```
    planet number of the interpolated lunar agopee. It is equal to 21.
    
    See Also:
    
    Constant Field Values
  - SE_INTP_PERG
```
public static final int SE_INTP_PERG
```
    planet number of the interpolated lunar perigee. It is equal to 22.
    
    See Also:
    
    Constant Field Values
  - SE_AST_OFFSET
```
public static final int SE_AST_OFFSET
```
    The offset, where asteroid numbers start. It is equal to 10000.
    
    See Also:
    
    Constant Field Values
  - SE_VARUNA
```
public static final int SE_VARUNA
```
    See Also:
    
    Constant Field Values
  - SE_FICT_OFFSET_1
```
public static final int SE_FICT_OFFSET_1
```
    See Also:
    
    Constant Field Values
  - SE_CUPIDO
```
public static final int SE_CUPIDO
```
    The number of the Hamburger or Uranian "planet" cupido. It is equal to 40.
    
    See Also:
    
    Constant Field Values
  - SE_HADES
```
public static final int SE_HADES
```
    The number of the Hamburger or Uranian "planet" hades. It is equal to 41.
    
    See Also:
    
    Constant Field Values
  - SE_ZEUS
```
public static final int SE_ZEUS
```
    The number of the Hamburger or Uranian "planet" zeus. It is equal to 42.
    
    See Also:
    
    Constant Field Values
  - SE_KRONOS
```
public static final int SE_KRONOS
```
    The number of the Hamburger or Uranian "planet" kronos. It is equal to 43.
    
    See Also:
    
    Constant Field Values
  - SE_APOLLON
```
public static final int SE_APOLLON
```
    The number of the Hamburger or Uranian "planet" appollon. It is equal to 44.
    
    See Also:
    
    Constant Field Values
  - SE_ADMETOS
```
public static final int SE_ADMETOS
```
    The number of the Hamburger or Uranian "planet" admetos. It is equal to 45.
    
    See Also:
    
    Constant Field Values
  - SE_VULKANUS
```
public static final int SE_VULKANUS
```
    The number of the Hamburger or Uranian "planet" vulkanus. It is equal to 46.
    
    See Also:
    
    Constant Field Values
  - SE_POSEIDON
```
public static final int SE_POSEIDON
```
    The number of the Hamburger or Uranian "planet" poseidon. It is equal to 47.
    
    See Also:
    
    Constant Field Values
  - SE_ISIS
```
public static final int SE_ISIS
```
    The "planet" number of the fictitious body isis. It is equal to 48.
    
    See Also:
    
    Constant Field Values
  - SE_NIBIRU
```
public static final int SE_NIBIRU
```
    The "planet" number of the fictitious body nibiru. It is equal to 49.
    
    See Also:
    
    Constant Field Values
  - SE_HARRINGTON
```
public static final int SE_HARRINGTON
```
    The "planet" number of the fictitious body harrington. It is equal to 50.
    
    See Also:
    
    Constant Field Values
  - SE_NEPTUNE_LEVERRIER
```
public static final int SE_NEPTUNE_LEVERRIER
```
    The "planet" number of the fictitious body neptune-leverrier. It is equal to 51.
    
    See Also:
    
    Constant Field Values
  - SE_NEPTUNE_ADAMS
```
public static final int SE_NEPTUNE_ADAMS
```
    The "planet" number of the fictitious body neptune-adams. It is equal to 52.
    
    See Also:
    
    Constant Field Values
  - SE_PLUTO_LOWELL
```
public static final int SE_PLUTO_LOWELL
```
    The "planet" number of the fictitious body pluto-lowell. It is equal to 53.
    
    See Also:
    
    Constant Field Values
  - SE_PLUTO_PICKERING
```
public static final int SE_PLUTO_PICKERING
```
    The "planet" number of the fictitious body pluto-pickering. It is equal to 54.
    
    See Also:
    
    Constant Field Values
  - SE_VULCAN
```
public static final int SE_VULCAN
```
    The "planet" number of the fictitious body vulcan. It is equal to 55.
    
    See Also:
    
    Constant Field Values
  - SE_WHITE_MOON
```
public static final int SE_WHITE_MOON
```
    The "planet" number of the fictitious body "white moon" (== Selena). It is equal to 56.
    
    See Also:
    
    Constant Field Values
  - SE_PROSERPINA
```
public static final int SE_PROSERPINA
```
    The "planet" number of the fictitious body "Proserpina". It is equal to 57.
    
    See Also:
    
    Constant Field Values
  - SE_WALDEMATH
```
public static final int SE_WALDEMATH
```
    The "planet" number of the fictitious body "Waldemath". It is equal to 58.
    
    See Also:
    
    Constant Field Values
  - SE_FIXSTAR
```
public static final int SE_FIXSTAR
```
    See Also:
    
    Constant Field Values
  - SE_ASC
```
public static final int SE_ASC
```
    This is a constant to access the ascendant value in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the ascendant object in transit calculations. Its value is 0.
    
    See Also:
    
    Constant Field Values
  - SE_MC
```
public static final int SE_MC
```
    This is a constant to access the medium coeli value in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the medium coeli object in transit calculations. Its value is 1.
    
    See Also:
    
    Constant Field Values
  - SE_ARMC
```
public static final int SE_ARMC
```
    This is a constant to access the value of the sidereal time in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the sidereal time as an object in transit calculations. Its value is 2.
    
    See Also:
    
    Constant Field Values
  - SE_VERTEX
```
public static final int SE_VERTEX
```
    This is a constant to access the vertex value in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the vertex object in transit calculations. Its value is 3.
    
    See Also:
    
    Constant Field Values
  - SE_EQUASC
```
public static final int SE_EQUASC
```
    This is a constant to access the value of the "equatorial ascendant" in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the equatorial ascendant object in transit calculations. Its value is 4.
    
    See Also:
    
    Constant Field Values
  - SE_COASC1
```
public static final int SE_COASC1
```
    This is a constant to access the value of the "co-ascendant" of W. Koch in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the corresponding object in transit calculations. Its value is 5.
    
    See Also:
    
    Constant Field Values
  - SE_COASC2
```
public static final int SE_COASC2
```
    This is a constant to access the value of the "co-ascendant" of M. Munkasey in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the corresponding object in transit calculations. Its value is 6.
    
    See Also:
    
    Constant Field Values
  - SE_POLASC
```
public static final int SE_POLASC
```
    This is a constant to access the polar ascendant value of M. Munkasey in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses() or to specify the corresponding object in transit calculations. Its value is 7.
    
    See Also:
    
    Constant Field Values
  - SE_NASCMC
```
public static final int SE_NASCMC
```
    This is a constant to know the count of valid parameters in parameter ascmc[] of SwissEph.swe_houses_armc() / SwissEph.swe_houses(). Its value is 8 now, meaning, ascmc[0] to ascmc[7] contain meaningful data, even though ascmc[] has to be of size 10.
    
    See Also:
    
    Constant Field Values
  - SE_DE_NUMBER
```
public static final int SE_DE_NUMBER
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DE200
```
public static final java.lang.String SE_FNAME_DE200
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DE403
```
public static final java.lang.String SE_FNAME_DE403
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DE404
```
public static final java.lang.String SE_FNAME_DE404
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DE405
```
public static final java.lang.String SE_FNAME_DE405
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DE406
```
public static final java.lang.String SE_FNAME_DE406
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DE431
```
public static final java.lang.String SE_FNAME_DE431
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DFT
```
public static final java.lang.String SE_FNAME_DFT
```
    See Also:
    
    Constant Field Values
  - SE_FNAME_DFT2
```
public static final java.lang.String SE_FNAME_DFT2
```
    See Also:
    
    Constant Field Values
  - SEFLG_HELCTR
```
public static final int SEFLG_HELCTR
```
    Calculate the heliocentric position of the planet. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_TRUEPOS
```
public static final int SEFLG_TRUEPOS
```
    Calculate the true position of the planet versus the apparent position. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_J2000
```
public static final int SEFLG_J2000
```
    Calculate the position of the planet without considering the precession, i.e., calculate J2000 equinox. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_NONUT
```
public static final int SEFLG_NONUT
```
    Calculate the position of the planet without considering the nutation, i.e., calculate the mean equinox of the day. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_SPEED3
```
public static final int SEFLG_SPEED3
```
    Calculate the speed of the planet. This calculation should not be used, as it is slower and less precise than SEFLG_SPEED. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    SEFLG_SPEED, Constant Field Values
  - SEFLG_SPEED
```
public static final int SEFLG_SPEED
```
    Calculate the speed of the planet. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_NOGDEFL
```
public static final int SEFLG_NOGDEFL
```
    Calculate the position of the planet without considering gravitational deflection. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_NOABERR
```
public static final int SEFLG_NOABERR
```
    Calculate the position of the planet without considering the 'annual' aberration of light. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_EQUATORIAL
```
public static final int SEFLG_EQUATORIAL
```
    Calculate the position of the planet in the earth equator coordinate system. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_XYZ
```
public static final int SEFLG_XYZ
```
    Return cartesian coordinates instead of polar coordinates. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_RADIANS
```
public static final int SEFLG_RADIANS
```
    Return coordinates in radians instead of degrees. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_BARYCTR
```
public static final int SEFLG_BARYCTR
```
    Calculate barycentric positions. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_TOPOCTR
```
public static final int SEFLG_TOPOCTR
```
    Calculate topocentric positions. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_SIDEREAL
```
public static final int SEFLG_SIDEREAL
```
    Calculate sidereal positions. This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SEFLG_ICRS
```
public static final int SEFLG_ICRS
```
    Calculate in the "International Celestial Reference System." This is a constant to be used as a flag to swe_calc() / swe_fixstar().
    
    See Also:
    
    Constant Field Values
  - SEFLG_DPSIDEPS_1980
```
public static final int SEFLG_DPSIDEPS_1980
```
    See Also:
    
    Constant Field Values
  - SEFLG_JPLHOR
```
public static final int SEFLG_JPLHOR
```
    See Also:
    
    Constant Field Values
  - SEFLG_JPLHOR_APPROX
```
public static final int SEFLG_JPLHOR_APPROX
```
    See Also:
    
    Constant Field Values
  - SEFLG_TRANSIT_LONGITUDE
```
public static final int SEFLG_TRANSIT_LONGITUDE
```
    calculate transits over a longitude. This is a constant to be used as a flag to the TransitCalculator constructors.
    
    See Also:
    
    TCPlanet.TCPlanet(SwissEph, int, int, double), TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), Constant Field Values
  - SEFLG_TRANSIT_LATITUDE
```
public static final int SEFLG_TRANSIT_LATITUDE
```
    calculate transits over a latitude. This is a constant to be used as a flag to the TransitCalculator constructors.
    
    See Also:
    
    TCPlanet.TCPlanet(SwissEph, int, int, double), TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), Constant Field Values
  - SEFLG_TRANSIT_DISTANCE
```
public static final int SEFLG_TRANSIT_DISTANCE
```
    calculate transits over a distance in AU. This is a constant to be used as a flag to the TransitCalculator constructors.
    
    See Also:
    
    TCPlanet.TCPlanet(SwissEph, int, int, double), TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), Constant Field Values
  - SEFLG_TRANSIT_SPEED
```
public static final int SEFLG_TRANSIT_SPEED
```
    calculate transits over a (longitudinal, latitudinal or distance) speed value. This is a constant to be used as a flag the TransitCalculator constructors.
    
    See Also:
    
    TCPlanet.TCPlanet(SwissEph, int, int, double), TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), Constant Field Values
  - SEFLG_YOGA_TRANSIT
```
public static final int SEFLG_YOGA_TRANSIT
```
    calculate yoga transits, this means consider the SUM of two planets positions or speeds instead of the difference. This is a constant to be used as a flag to the TransitCalculator constructors.
    
    See Also:
    
    TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), Constant Field Values
  - SEFLG_PARTILE_TRANSIT_START
```
public static final int SEFLG_PARTILE_TRANSIT_START
```
    calculate partile transits. This calculates the times when two planets have an identically integer degree value in their respective sign == 30 degree section: (int)(lon1 % 30) == (int)(lon2 % 30). This is a flag to the TransitCalculator constructors.
    
    See Also:
    
    TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), Constant Field Values
  - SEFLG_PARTILE_TRANSIT_END
```
public static final int SEFLG_PARTILE_TRANSIT_END
```
    calculate partile transits. This calculates the time when two planets aren't partile anymore. So they don't have an identically integer degree value in their respective sign == 30 degree section: (int)(lon1 % 30) != (int)(lon2 % 30). This is a flag to the TransitCalculator constructors.
    
    See Also:
    
    TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), Constant Field Values
  - SEFLG_PARTILE_TRANSIT
```
public static final int SEFLG_PARTILE_TRANSIT
```
    calculate partile transits. This calculates the time when two planets gain or loose a partile aspect, depending on if they have a partile aspect on the starting date or not. This is a flag to the TransitCalculator constructors.
    
    See Also:
    
    TCPlanetPlanet.TCPlanetPlanet(SwissEph, int, int, int, double), SEFLG_PARTILE_TRANSIT_START, SEFLG_PARTILE_TRANSIT_END, Constant Field Values
  - SE_HOUSE1
```
public static final int SE_HOUSE1
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE2
```
public static final int SE_HOUSE2
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE3
```
public static final int SE_HOUSE3
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE4
```
public static final int SE_HOUSE4
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE5
```
public static final int SE_HOUSE5
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE6
```
public static final int SE_HOUSE6
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE7
```
public static final int SE_HOUSE7
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE8
```
public static final int SE_HOUSE8
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE9
```
public static final int SE_HOUSE9
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE10
```
public static final int SE_HOUSE10
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE11
```
public static final int SE_HOUSE11
```
    See Also:
    
    Constant Field Values
  - SE_HOUSE12
```
public static final int SE_HOUSE12
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_PLACIDUS
```
public static final int SE_HSYS_PLACIDUS
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_KOCH
```
public static final int SE_HSYS_KOCH
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_PORPHYRIUS
```
public static final int SE_HSYS_PORPHYRIUS
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_REGIOMONTANUS
```
public static final int SE_HSYS_REGIOMONTANUS
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_CAMPANUS
```
public static final int SE_HSYS_CAMPANUS
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_EQUAL
```
public static final int SE_HSYS_EQUAL
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_VEHLOW
```
public static final int SE_HSYS_VEHLOW
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_MERIDIAN
```
public static final int SE_HSYS_MERIDIAN
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_HORIZONTAL
```
public static final int SE_HSYS_HORIZONTAL
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_POLICH_PAGE
```
public static final int SE_HSYS_POLICH_PAGE
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_ALCABITIUS
```
public static final int SE_HSYS_ALCABITIUS
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_GAUQUELIN_SECTORS
```
public static final int SE_HSYS_GAUQUELIN_SECTORS
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_MORINUS
```
public static final int SE_HSYS_MORINUS
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_KRUSINSKI
```
public static final int SE_HSYS_KRUSINSKI
```
    See Also:
    
    Constant Field Values
  - SE_HSYS_WHOLE_SIGN
```
public static final int SE_HSYS_WHOLE_SIGN
```
    See Also:
    
    Constant Field Values
  - SEFLG_JPLEPH
```
public static final int SEFLG_JPLEPH
```
    Use the calculation routines that use the ephemeris data files of the Solar System Dynamics Group of the Jet Propulsion Laboratory of NASA http://ssd.jpl.nasa.gov/. This requires you to have the ephemeris data files from JPL (DE406: about 9.5 MB per 300 years). They can be obtained from ftp://navigator.jpl.nasa.gov/pub/ephem/export (as of December 21, 2000).
    
    See Also:
    
    SwissEph.swe_set_ephe_path(java.lang.String), Constant Field Values
  - SEFLG_SWIEPH
```
public static final int SEFLG_SWIEPH
```
    Use the calculation routines of Swiss Ephemeris from Astrodienst AG Zürich http://www.astro.com. This requires you to have the data files for SwissEphemeris available and in the search path for the ephemeris files.
    Basically, these routines are identical to the JPL routines, but the data files are much more compressed (about one 10th of the original JPL files), and the exactness is retained to 1/1000 of an arc second.
    
    See Also:
    
    SwissEph.swe_set_ephe_path(java.lang.String), Constant Field Values
  - SEFLG_MOSEPH
```
public static final int SEFLG_MOSEPH
```
    Use the Moshier semi-analytical calculation routines. These routines are the slowest (about 10 times slower than JPL or SWISS EPHEMERIS) and most inaccurate, but they do not require any additional data files.
    The accuracy is about 1 arc seconds for the planets and a few arc seconds for the moon. Unfortunately, the deviation for true lunar nodes may be up to one arc minute.
    
    See Also:
    
    Constant Field Values
  - SEFLG_DEFAULTEPH
```
public static final int SEFLG_DEFAULTEPH
```
    Defines the default method of calculation as SEFLG_SWIEPH.
    
    See Also:
    
    SEFLG_JPLEPH, SEFLG_SWIEPH, SEFLG_MOSEPH, Constant Field Values
  - SEFLG_EPHMASK
```
public static final int SEFLG_EPHMASK
```
    See Also:
    
    Constant Field Values
  - SE_SIDBITS
```
public static final int SE_SIDBITS
```
    See Also:
    
    Constant Field Values
  - SE_SIDBIT_ECL_T0
```
public static final int SE_SIDBIT_ECL_T0
```
    This specifies that sidereal calculations are done via a projection onto the ecliptic at date t0.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDBIT_SSY_PLANE
```
public static final int SE_SIDBIT_SSY_PLANE
```
    This specifies that sidereal calculations are done via a projection onto the solar system plane.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_FAGAN_BRADLEY
```
public static final int SE_SIDM_FAGAN_BRADLEY
```
    A constant to be used for specifying the sidereal mode (ayanamsha). Fagan/Bradley is used as default, if nothing other is specified via swe_set_sid_mode.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_LAHIRI
```
public static final int SE_SIDM_LAHIRI
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Lahiri.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_DELUCE
```
public static final int SE_SIDM_DELUCE
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by De Luce.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_RAMAN
```
public static final int SE_SIDM_RAMAN
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Raman.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_USHASHASHI
```
public static final int SE_SIDM_USHASHASHI
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Ushashashi.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_KRISHNAMURTI
```
public static final int SE_SIDM_KRISHNAMURTI
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Krishnamurti.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_DJWHAL_KHUL
```
public static final int SE_SIDM_DJWHAL_KHUL
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Djwhal Khool.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_YUKTESHWAR
```
public static final int SE_SIDM_YUKTESHWAR
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Sri Yukteshwar.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_JN_BHASIN
```
public static final int SE_SIDM_JN_BHASIN
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by JN Bhasin.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_BABYL_KUGLER1
```
public static final int SE_SIDM_BABYL_KUGLER1
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Kugler 1.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_BABYL_KUGLER2
```
public static final int SE_SIDM_BABYL_KUGLER2
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Kugler 2.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_BABYL_KUGLER3
```
public static final int SE_SIDM_BABYL_KUGLER3
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Kugler 3.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_BABYL_HUBER
```
public static final int SE_SIDM_BABYL_HUBER
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Huber.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_BABYL_ETPSC
```
public static final int SE_SIDM_BABYL_ETPSC
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Babylonian, Mercier.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_ALDEBARAN_15TAU
```
public static final int SE_SIDM_ALDEBARAN_15TAU
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defining t0 by Aldebaran at 15 degrees Taurus.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_HIPPARCHOS
```
public static final int SE_SIDM_HIPPARCHOS
```
    A constant to be used for specifying the sidereal mode (ayanamsha) by defined by Hipparchos.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_SASSANIAN
```
public static final int SE_SIDM_SASSANIAN
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by Sassanian.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_GALCENT_0SAG
```
public static final int SE_SIDM_GALCENT_0SAG
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by the galactic center being at 0 degrees Sagittarius.
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_J2000
```
public static final int SE_SIDM_J2000
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as J2000 (Julian day 2451545.0, 2000 January 1.5)
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_J1900
```
public static final int SE_SIDM_J1900
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as J1900 (Julian day 2415020.0, 1900 January 0.5).
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_B1950
```
public static final int SE_SIDM_B1950
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as B1950 (Julian day 2433282.42345905, 1950 January 0.923).
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_SURYASIDDHANTA
```
public static final int SE_SIDM_SURYASIDDHANTA
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as SURYASIDDHANTA (Suryasiddhanta, assuming ingress of mean Sun into Aries at point of mean equinox of date on 21.3.499, noon, Ujjain (75.7684565 E) = 7:30:31.57 UT).
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_SURYASIDDHANTA_MSUN
```
public static final int SE_SIDM_SURYASIDDHANTA_MSUN
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as SURYASIDDHANTA_MSUN (Suryasiddhanta, assuming ingress of mean Sun into Aries at true position of mean Sun at same epoch).
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_ARYABHATA
```
public static final int SE_SIDM_ARYABHATA
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as ARYABHATA (Aryabhata, same date as SE_SIDM_SURYASIDDHANTA_MSUN, but UT 6:56:55.57).
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_ARYABHATA_MSUN
```
public static final int SE_SIDM_ARYABHATA_MSUN
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as ARYABHATA_MSUN (Aryabhata, analogous SE_SIDM_SURYASIDDHANTA_MSUN).
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_SS_REVATI
```
public static final int SE_SIDM_SS_REVATI
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_SS_REVATI (SS, Revati/zePsc at polar long. 359°50').
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_SS_CITRA
```
public static final int SE_SIDM_SS_CITRA
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_SS_CITRA (SS, Citra/Spica at polar long. 180°).
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_TRUE_CITRA
```
public static final int SE_SIDM_TRUE_CITRA
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_TRUE_CITRA (True Spica (Spica exactly at 0 Libra)
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_TRUE_REVATI
```
public static final int SE_SIDM_TRUE_REVATI
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_TRUE_REVATI (True Revati (zeta Psc exactly at 0 Aries))
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_TRUE_PUSHYA
```
public static final int SE_SIDM_TRUE_PUSHYA
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as SE_SIDM_TRUE_PUSHYA (True Pushya (delta Cnc exactly a 16 Cancer))
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_SIDM_USER
```
public static final int SE_SIDM_USER
```
    A constant to be used for specifying the sidereal mode (ayanamsha) as defined by the user in the additional two parameters of swe_set_sid_mode().
    
    See Also:
    
    SwissEph.swe_set_sid_mode(int, double, double), Constant Field Values
  - SE_NODBIT_MEAN
```
public static final int SE_NODBIT_MEAN
```
    Used for swe_nod_aps(): mean nodes/apsides
    
    See Also:
    
    Constant Field Values
  - SE_NODBIT_OSCU
```
public static final int SE_NODBIT_OSCU
```
    Used for swe_nod_aps(): osculating nodes/apsides
    
    See Also:
    
    Constant Field Values
  - SE_NODBIT_OSCU_BAR
```
public static final int SE_NODBIT_OSCU_BAR
```
    Used for swe_nod_aps(): osculating nodes/apsides, but motion about solar system barycenter is considered
    
    See Also:
    
    Constant Field Values
  - SE_NODBIT_FOPOINT
```
public static final int SE_NODBIT_FOPOINT
```
    Used for swe_nod_aps(): focal point of orbit instead of aphelion
    
    See Also:
    
    Constant Field Values
  - SE_SPLIT_DEG_ROUND_SEC
```
public static final int SE_SPLIT_DEG_ROUND_SEC
```
    See Also:
    
    Constant Field Values
  - SE_SPLIT_DEG_ROUND_MIN
```
public static final int SE_SPLIT_DEG_ROUND_MIN
```
    See Also:
    
    Constant Field Values
  - SE_SPLIT_DEG_ROUND_DEG
```
public static final int SE_SPLIT_DEG_ROUND_DEG
```
    See Also:
    
    Constant Field Values
  - SE_SPLIT_DEG_ZODIACAL
```
public static final int SE_SPLIT_DEG_ZODIACAL
```
    See Also:
    
    Constant Field Values
  - SE_SPLIT_DEG_KEEP_SIGN
```
public static final int SE_SPLIT_DEG_KEEP_SIGN
```
    SwissLib.swe_split_deg(): Don't round to next sign, e.g. 29.9999999 will be rounded to 29d59'59" (or 29d59' or 29d)
    
    See Also:
    
    Constant Field Values
  - SE_SPLIT_DEG_KEEP_DEG
```
public static final int SE_SPLIT_DEG_KEEP_DEG
```
    SwissLib.swe_split_deg(): Don't round to next degree, e.g. 13.9999999 will be rounded to 13d59'59" (or 13d59' or 13d)
    
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_RISING
```
public static final int SE_HELIACAL_RISING
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_SETTING
```
public static final int SE_HELIACAL_SETTING
```
    See Also:
    
    Constant Field Values
  - SE_MORNING_FIRST
```
public static final int SE_MORNING_FIRST
```
    See Also:
    
    Constant Field Values
  - SE_EVENING_LAST
```
public static final int SE_EVENING_LAST
```
    See Also:
    
    Constant Field Values
  - SE_EVENING_FIRST
```
public static final int SE_EVENING_FIRST
```
    See Also:
    
    Constant Field Values
  - SE_MORNING_LAST
```
public static final int SE_MORNING_LAST
```
    See Also:
    
    Constant Field Values
  - SE_ACRONYCHAL_RISING
```
public static final int SE_ACRONYCHAL_RISING
```
    See Also:
    
    Constant Field Values
  - SE_ACRONYCHAL_SETTING
```
public static final int SE_ACRONYCHAL_SETTING
```
    See Also:
    
    Constant Field Values
  - SE_COSMICAL_SETTING
```
public static final int SE_COSMICAL_SETTING
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_LONG_SEARCH
```
public static final int SE_HELFLAG_LONG_SEARCH
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_HIGH_PRECISION
```
public static final int SE_HELFLAG_HIGH_PRECISION
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_OPTICAL_PARAMS
```
public static final int SE_HELFLAG_OPTICAL_PARAMS
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_NO_DETAILS
```
public static final int SE_HELFLAG_NO_DETAILS
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_SEARCH_1_PERIOD
```
public static final int SE_HELFLAG_SEARCH_1_PERIOD
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_VISLIM_DARK
```
public static final int SE_HELFLAG_VISLIM_DARK
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_VISLIM_NOMOON
```
public static final int SE_HELFLAG_VISLIM_NOMOON
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_VISLIM_PHOTOPIC
```
public static final int SE_HELFLAG_VISLIM_PHOTOPIC
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_AV
```
public static final int SE_HELFLAG_AV
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_AVKIND_VR
```
public static final int SE_HELFLAG_AVKIND_VR
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_AVKIND_PTO
```
public static final int SE_HELFLAG_AVKIND_PTO
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_AVKIND_MIN7
```
public static final int SE_HELFLAG_AVKIND_MIN7
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_AVKIND_MIN9
```
public static final int SE_HELFLAG_AVKIND_MIN9
```
    See Also:
    
    Constant Field Values
  - SE_HELFLAG_AVKIND
```
public static final int SE_HELFLAG_AVKIND
```
    See Also:
    
    Constant Field Values
  - TJD_INVALID
```
public static final double TJD_INVALID
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_LONG_SEARCH
```
public static final int SE_HELIACAL_LONG_SEARCH
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_HIGH_PRECISION
```
public static final int SE_HELIACAL_HIGH_PRECISION
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_OPTICAL_PARAMS
```
public static final int SE_HELIACAL_OPTICAL_PARAMS
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_NO_DETAILS
```
public static final int SE_HELIACAL_NO_DETAILS
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_SEARCH_1_PERIOD
```
public static final int SE_HELIACAL_SEARCH_1_PERIOD
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_VISLIM_DARK
```
public static final int SE_HELIACAL_VISLIM_DARK
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_VISLIM_NOMOON
```
public static final int SE_HELIACAL_VISLIM_NOMOON
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_VISLIM_PHOTOPIC
```
public static final int SE_HELIACAL_VISLIM_PHOTOPIC
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_AVKIND_VR
```
public static final int SE_HELIACAL_AVKIND_VR
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_AVKIND_PTO
```
public static final int SE_HELIACAL_AVKIND_PTO
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_AVKIND_MIN7
```
public static final int SE_HELIACAL_AVKIND_MIN7
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_AVKIND_MIN9
```
public static final int SE_HELIACAL_AVKIND_MIN9
```
    See Also:
    
    Constant Field Values
  - SE_HELIACAL_AVKIND
```
public static final int SE_HELIACAL_AVKIND
```
    See Also:
    
    Constant Field Values
  - SE_PHOTOPIC_FLAG
```
public static final int SE_PHOTOPIC_FLAG
```
    See Also:
    
    Constant Field Values
  - SE_SCOTOPIC_FLAG
```
public static final int SE_SCOTOPIC_FLAG
```
    See Also:
    
    Constant Field Values
  - SE_MIXEDOPIC_FLAG
```
public static final int SE_MIXEDOPIC_FLAG
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE200
```
public static final double SE_TIDAL_DE200
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE403
```
public static final double SE_TIDAL_DE403
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE404
```
public static final double SE_TIDAL_DE404
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE405
```
public static final double SE_TIDAL_DE405
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE406
```
public static final double SE_TIDAL_DE406
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE421
```
public static final double SE_TIDAL_DE421
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE430
```
public static final double SE_TIDAL_DE430
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DE431
```
public static final double SE_TIDAL_DE431
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_26
```
public static final double SE_TIDAL_26
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_DEFAULT
```
public static final double SE_TIDAL_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_AUTOMATIC
```
public static final double SE_TIDAL_AUTOMATIC
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_MOSEPH
```
public static final double SE_TIDAL_MOSEPH
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_SWIEPH
```
public static final double SE_TIDAL_SWIEPH
```
    See Also:
    
    Constant Field Values
  - SE_TIDAL_JPLEPH
```
public static final double SE_TIDAL_JPLEPH
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_PREC_LONGTERM
```
public static final int SE_MODEL_PREC_LONGTERM
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_PREC_SHORTTERM
```
public static final int SE_MODEL_PREC_SHORTTERM
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_NUT
```
public static final int SE_MODEL_NUT
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_SIDT
```
public static final int SE_MODEL_SIDT
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_BIAS
```
public static final int SE_MODEL_BIAS
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_JPLHOR_MODE
```
public static final int SE_MODEL_JPLHOR_MODE
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_JPLHORA_MODE
```
public static final int SE_MODEL_JPLHORA_MODE
```
    See Also:
    
    Constant Field Values
  - SE_MODEL_DELTAT
```
public static final int SE_MODEL_DELTAT
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_IAU_1976
```
public static final int SEMOD_PREC_IAU_1976
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_IAU_2000
```
public static final int SEMOD_PREC_IAU_2000
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_IAU_2006
```
public static final int SEMOD_PREC_IAU_2006
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_BRETAGNON_2003
```
public static final int SEMOD_PREC_BRETAGNON_2003
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_LASKAR_1986
```
public static final int SEMOD_PREC_LASKAR_1986
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_SIMON_1994
```
public static final int SEMOD_PREC_SIMON_1994
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_WILLIAMS_1994
```
public static final int SEMOD_PREC_WILLIAMS_1994
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_VONDRAK_2011
```
public static final int SEMOD_PREC_VONDRAK_2011
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_DEFAULT
```
public static final int SEMOD_PREC_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SEMOD_PREC_DEFAULT_SHORT
```
public static final int SEMOD_PREC_DEFAULT_SHORT
```
    See Also:
    
    Constant Field Values
  - SEMOD_NUT_IAU_1980
```
public static final int SEMOD_NUT_IAU_1980
```
    See Also:
    
    Constant Field Values
  - SEMOD_NUT_IAU_CORR_1987
```
public static final int SEMOD_NUT_IAU_CORR_1987
```
    See Also:
    
    Constant Field Values
  - SEMOD_NUT_IAU_2000A
```
public static final int SEMOD_NUT_IAU_2000A
```
    See Also:
    
    Constant Field Values
  - SEMOD_NUT_IAU_2000B
```
public static final int SEMOD_NUT_IAU_2000B
```
    See Also:
    
    Constant Field Values
  - SEMOD_NUT_DEFAULT
```
public static final int SEMOD_NUT_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SEMOD_SIDT_LONGTERM
```
public static final int SEMOD_SIDT_LONGTERM
```
    See Also:
    
    Constant Field Values
  - SEMOD_SIDT_IERS_CONV_2010
```
public static final int SEMOD_SIDT_IERS_CONV_2010
```
    See Also:
    
    Constant Field Values
  - SEMOD_SIDT_PREC_MODEL
```
public static final int SEMOD_SIDT_PREC_MODEL
```
    See Also:
    
    Constant Field Values
  - SEMOD_SIDT_DEFAULT
```
public static final int SEMOD_SIDT_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SEMOD_BIAS_IAU2000
```
public static final int SEMOD_BIAS_IAU2000
```
    See Also:
    
    Constant Field Values
  - SEMOD_BIAS_IAU2006
```
public static final int SEMOD_BIAS_IAU2006
```
    See Also:
    
    Constant Field Values
  - SEMOD_BIAS_DEFAULT
```
public static final int SEMOD_BIAS_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SEMOD_JPLHOR_EXTENDED_1800
```
public static final int SEMOD_JPLHOR_EXTENDED_1800
```
    See Also:
    
    Constant Field Values
  - SEMOD_JPLHOR_NOT_EXTENDED
```
public static final int SEMOD_JPLHOR_NOT_EXTENDED
```
    See Also:
    
    Constant Field Values
  - SEMOD_JPLHOR_DEFAULT
```
public static final int SEMOD_JPLHOR_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SEMOD_JPLHORA_1
```
public static final int SEMOD_JPLHORA_1
```
    See Also:
    
    Constant Field Values
  - SEMOD_JPLHORA_2
```
public static final int SEMOD_JPLHORA_2
```
    See Also:
    
    Constant Field Values
  - SEMOD_JPLHORA_DEFAULT
```
public static final int SEMOD_JPLHORA_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SEMOD_DELTAT_ESPENAK_MEEUS_2006
```
public static final int SEMOD_DELTAT_ESPENAK_MEEUS_2006
```
    See Also:
    
    Constant Field Values
  - SEMOD_DELTAT_STEPHENSON_MORRISON_2004
```
public static final int SEMOD_DELTAT_STEPHENSON_MORRISON_2004
```
    See Also:
    
    Constant Field Values
  - SEMOD_DELTAT_DEFAULT
```
public static final int SEMOD_DELTAT_DEFAULT
```
    See Also:
    
    Constant Field Values
  - SE_EPHE_PATH
```
public static final java.lang.String SE_EPHE_PATH
```
    Ephemeris path.
    This defines where ephemeris files are expected if the function swe_set_ephe_path() is not called by the application.
    It is defined as being ".:./ephe:/users/ephe2/:/users/ephe/".
    
    See Also:
    
    SwissEph.swe_set_ephe_path(java.lang.String), Constant Field Values
  - SE_ECL_CENTRAL
```
public static final int SE_ECL_CENTRAL
```
    See Also:
    
    Constant Field Values
  - SE_ECL_NONCENTRAL
```
public static final int SE_ECL_NONCENTRAL
```
    See Also:
    
    Constant Field Values
  - SE_ECL_TOTAL
```
public static final int SE_ECL_TOTAL
```
    See Also:
    
    Constant Field Values
  - SE_ECL_ANNULAR
```
public static final int SE_ECL_ANNULAR
```
    Annular eclipse. This is an eclipse, where the moon is seen smaller than the sun, so you get a "ring" of the sun around the moon.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_PARTIAL
```
public static final int SE_ECL_PARTIAL
```
    See Also:
    
    Constant Field Values
  - SE_ECL_ANNULAR_TOTAL
```
public static final int SE_ECL_ANNULAR_TOTAL
```
    See Also:
    
    Constant Field Values
  - SE_ECL_PENUMBRAL
```
public static final int SE_ECL_PENUMBRAL
```
    See Also:
    
    Constant Field Values
  - SE_ECL_ALLTYPES_SOLAR
```
public static final int SE_ECL_ALLTYPES_SOLAR
```
    See Also:
    
    Constant Field Values
  - SE_ECL_ALLTYPES_LUNAR
```
public static final int SE_ECL_ALLTYPES_LUNAR
```
    See Also:
    
    Constant Field Values
  - SE_ECL_VISIBLE
```
public static final int SE_ECL_VISIBLE
```
    See Also:
    
    Constant Field Values
  - SE_ECL_MAX_VISIBLE
```
public static final int SE_ECL_MAX_VISIBLE
```
    See Also:
    
    Constant Field Values
  - SE_ECL_1ST_VISIBLE
```
public static final int SE_ECL_1ST_VISIBLE
```
    Begin of partial eclipse. This is the time, when the moon touches the sun the first time.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_PARTBEG_VISIBLE
```
public static final int SE_ECL_PARTBEG_VISIBLE
```
    Begin of partial eclipse. This is the time, when the moon touches the sun the first time.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_2ND_VISIBLE
```
public static final int SE_ECL_2ND_VISIBLE
```
    Begin of total eclipse. This is the time, when the sun completely disappears.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_TOTBEG_VISIBLE
```
public static final int SE_ECL_TOTBEG_VISIBLE
```
    Begin of total eclipse. This is the time, when the sun completely disappears.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_3RD_VISIBLE
```
public static final int SE_ECL_3RD_VISIBLE
```
    End of total eclipse. This is the time, when the sun starts to reappear.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_TOTEND_VISIBLE
```
public static final int SE_ECL_TOTEND_VISIBLE
```
    End of total eclipse. This is the time, when the sun starts to reappear.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_4TH_VISIBLE
```
public static final int SE_ECL_4TH_VISIBLE
```
    End of partial eclipse. This is the time, when the moon and the sun finally separate.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_PARTEND_VISIBLE
```
public static final int SE_ECL_PARTEND_VISIBLE
```
    End of partial eclipse. This is the time, when the moon and the sun finally separate.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_PENUMBBEG_VISIBLE
```
public static final int SE_ECL_PENUMBBEG_VISIBLE
```
    Begin of penumbral eclipse.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_PENUMBEND_VISIBLE
```
public static final int SE_ECL_PENUMBEND_VISIBLE
```
    End of penumbral eclipse.
    
    See Also:
    
    Constant Field Values
  - SE_ECL_OCC_BEG_DAYLIGHT
```
public static final int SE_ECL_OCC_BEG_DAYLIGHT
```
    Occultation begins during the day
    
    See Also:
    
    Constant Field Values
  - SE_ECL_OCC_END_DAYLIGHT
```
public static final int SE_ECL_OCC_END_DAYLIGHT
```
    Occultation ends during the day
    
    See Also:
    
    Constant Field Values
  - SE_ECL_ONE_TRY
```
public static final int SE_ECL_ONE_TRY
```
    Just check if the next conjunction of the moon with a planet is an occultation; don't search further.
    
    See Also:
    
    Constant Field Values
  - SE_CALC_RISE
```
public static final int SE_CALC_RISE
```
    Calculate the time of sunrise. This is a constant to be used as a flag to swe_rise_trans().
    
    See Also:
    
    Constant Field Values
  - SE_CALC_SET
```
public static final int SE_CALC_SET
```
    Calculate the time of sunset. This is a constant to be used as a flag to swe_rise_trans().
    
    See Also:
    
    Constant Field Values
  - SE_CALC_MTRANSIT
```
public static final int SE_CALC_MTRANSIT
```
    Calculate the time of the upper meridian transit (southern for northern geo. latitudes). This is a constant to be used as a flag to swe_rise_trans().
    
    See Also:
    
    Constant Field Values
  - SE_CALC_ITRANSIT
```
public static final int SE_CALC_ITRANSIT
```
    Calculate the time of the lower meridian transit (northern, below the horizon). This is a constant to be used as a flag to swe_rise_trans().
    
    See Also:
    
    Constant Field Values
  - SE_BIT_DISC_CENTER
```
public static final int SE_BIT_DISC_CENTER
```
    Add this to SE_CALC_RISE/SET, if rise or set of disc center is requested. This is a constant to be used as a flag to swe_rise_trans().
    
    See Also:
    
    SwissEph.swe_rise_trans(double, int, java.lang.StringBuffer, int, int, double[], double, double, swisseph.DblObj, java.lang.StringBuffer), Constant Field Values
  - SE_BIT_DISC_BOTTOM
```
public static final int SE_BIT_DISC_BOTTOM
```
    Add this to SE_CALC_RISE/SET, if rise or set of disc bottom is requested. This is a constant to be used as a flag to swe_rise_trans().
    
    See Also:
    
    SwissEph.swe_rise_trans(double, int, java.lang.StringBuffer, int, int, double[], double, double, swisseph.DblObj, java.lang.StringBuffer), Constant Field Values
  - SE_BIT_NO_REFRACTION
```
public static final int SE_BIT_NO_REFRACTION
```
    Add this to SE_CALC_RISE/SET, if refraction should not to be considered. This is a constant to be used as a flag to swe_rise_trans().
    
    See Also:
    
    SwissEph.swe_rise_trans(double, int, java.lang.StringBuffer, int, int, double[], double, double, swisseph.DblObj, java.lang.StringBuffer), Constant Field Values
  - SE_BIT_CIVIL_TWILIGHT
```
public static final int SE_BIT_CIVIL_TWILIGHT
```
    See Also:
    
    Constant Field Values
  - SE_BIT_NAUTIC_TWILIGHT
```
public static final int SE_BIT_NAUTIC_TWILIGHT
```
    See Also:
    
    Constant Field Values
  - SE_BIT_ASTRO_TWILIGHT
```
public static final int SE_BIT_ASTRO_TWILIGHT
```
    See Also:
    
    Constant Field Values
  - SE_BIT_FIXED_DISC_SIZE
```
public static final int SE_BIT_FIXED_DISC_SIZE
```
    See Also:
    
    Constant Field Values
  - SE_ECL2HOR
```
public static final int SE_ECL2HOR
```
    This is a constant to be used as a flag to swe_azalt(). It determines the meaning of the contents of parameter xin[]. xin[0]= ecl. long., xin[1]= ecl. lat.. xin[2]=distance is not required.
    
    See Also:
    
    SwissEph.swe_azalt(double, int, double[], double, double, double[], double[]), Constant Field Values
  - SE_EQU2HOR
```
public static final int SE_EQU2HOR
```
    This is a constant to be used as a flag to swe_azalt(). It determines the meaning of the contents of parameter xin[]. xin[0]= rectascension, xin[1]= declination. xin[2]=distance is not required.
    
    See Also:
    
    SwissEph.swe_azalt(double, int, double[], double, double, double[], double[]), Constant Field Values
  - SE_HOR2ECL
```
public static final int SE_HOR2ECL
```
    This is a constant to be used as a flag to swe_azalt_rev(). It determines the meaning of the contents of output parameter xout[]. xout[0]= ecl. long., xout[1]= ecl. lat..
    
    See Also:
    
    SwissEph.swe_azalt_rev(double, int, double[], double[], double[]), Constant Field Values
  - SE_HOR2EQU
```
public static final int SE_HOR2EQU
```
    This is a constant to be used as a flag to swe_azalt_rev(). It determines the meaning of the contents of output parameter xout[]. xout[0]= equatorial long., xout[1]= equatorial lat..
    
    See Also:
    
    SwissEph.swe_azalt_rev(double, int, double[], double[], double[]), Constant Field Values
  - SE_TRUE_TO_APP
```
public static final int SE_TRUE_TO_APP
```
    Calculate the apparent altitude from the true altitude. This is a constant to be used as a flag to swe_refrac().
    
    See Also:
    
    SwissEph.swe_refrac(double, double, double, int), SE_APP_TO_TRUE, Constant Field Values
  - SE_APP_TO_TRUE
```
public static final int SE_APP_TO_TRUE
```
    Calculate the true altitude from the apparent altitude. This is a constant to be used as a flag to swe_refrac().
    
    See Also:
    
    SE_TRUE_TO_APP, SwissEph.swe_refrac(double, double, double, int), Constant Field Values
  - AUNIT
```
public static final double AUNIT
```
    See Also:
    
    Constant Field Values

Class SweConst

Field Summary

Method Summary

Methods inherited from class java.lang.Object

Field Detail

OK

ERR

SE_ECL_NUT

SE_SUN

SE_MOON

SE_MERCURY

SE_VENUS

SE_MARS

SE_JUPITER

SE_SATURN

SE_URANUS

SE_NEPTUNE

SE_PLUTO

SE_MEAN_NODE

SE_TRUE_NODE

SE_MEAN_APOG

SE_OSCU_APOG

SE_EARTH

SE_CHIRON

SE_PHOLUS

SE_CERES

SE_PALLAS

SE_JUNO

SE_VESTA

SE_INTP_APOG

SE_INTP_PERG

SE_AST_OFFSET

SE_VARUNA

SE_FICT_OFFSET_1

SE_CUPIDO

SE_HADES

SE_ZEUS

SE_KRONOS

SE_APOLLON

SE_ADMETOS

SE_VULKANUS

SE_POSEIDON

SE_ISIS

SE_NIBIRU

SE_HARRINGTON

SE_NEPTUNE_LEVERRIER

SE_NEPTUNE_ADAMS

SE_PLUTO_LOWELL

SE_PLUTO_PICKERING

SE_VULCAN

SE_WHITE_MOON

SE_PROSERPINA

SE_WALDEMATH

SE_FIXSTAR

SE_ASC

SE_MC

SE_ARMC

SE_VERTEX

SE_EQUASC

SE_COASC1

SE_COASC2

SE_POLASC

SE_NASCMC

SE_DE_NUMBER

SE_FNAME_DE200

SE_FNAME_DE403

SE_FNAME_DE404

SE_FNAME_DE405

SE_FNAME_DE406

SE_FNAME_DE431

SE_FNAME_DFT

SE_FNAME_DFT2

SEFLG_HELCTR

SEFLG_TRUEPOS

SEFLG_J2000

SEFLG_NONUT

SEFLG_SPEED3

SEFLG_SPEED

SEFLG_NOGDEFL

SEFLG_NOABERR