Uses of Class
edu.pdx.starview.calc.SVAngle

Packages that use SVAngle

edu.pdx.starview.calc
edu.pdx.starview.data
edu.pdx.starview.imaging
edu.pdx.starview.planets

Uses of SVAngle in edu.pdx.starview.calc

Fields in edu.pdx.starview.calc declared as SVAngle

SVAngle	SVAzAlt.azimuth The azimuth represented in radians.
SVAngle	SVAzAlt.altitude The altitude above the horizon represneted in radians.
SVAngle	SVRADec.RA The right ascention in the equatorial choord system.
SVAngle	SVRADec.Dec The decliation in the equatorial choord system.

Methods in edu.pdx.starview.calc that return SVAngle

SVAngle	KSNumbers.obliquity()
SVAngle	KSNumbers.constAberr()
SVAngle	KSNumbers.sunMeanAnomaly()
SVAngle	KSNumbers.sunMeanLongitude()
SVAngle	KSNumbers.sunTrueAnomaly()
SVAngle	KSNumbers.sunTrueLongitude()
SVAngle	KSNumbers.earthPerihelionLongitude()
SVAngle	KSSkyPoint.ra()
SVAngle	KSSkyPoint.dec()
SVAngle	SVAngle.getReducedDiff(SVAngle rhs)
SVAngle	SVAngle.getDiff(SVAngle rhs)
SVAngle	SVAzAlt.getAltitudeDMS()
SVAngle	SVAzAlt.getAzimuthDMS()
SVAngle	SVRADec.getRightAscensionDMS()
SVAngle	SVRADec.getDeclinationDMS()
static SVAngle	SVTime.getLocalSidrealTime(double julianDate, SVAngle longitude) TODO Make this compensate for nutation in longitude, the web page tells how to do this Note: Setting longitude to 0 (zero) will return greenwhich sidreal time http://aa.usno.navy.mil/faq/docs/GAST.html This is accurate to +/- 1.5 arcseconds

Methods in edu.pdx.starview.calc with parameters of type SVAngle

void	KSNumbers.getDeclAnddObq(SVAngle outdEcl, SVAngle outdObq) Returns the nutition in longitude and obliquity
void	KSSkyPoint.set(SVAngle r, SVAngle d) Sets RA, Dec and RA0, Dec0 according to arguments.
static void	KSSkyPoint.findEcliptic(SVAngle Obliquity, SVAngle EcLong, SVAngle EcLat, SVAngle RA, SVAngle Dec) Determine the Ecliptic coordinates of the SkyPoint, given the Julian Date.
static void	KSSkyPoint.setFromEcliptic(SVAngle Obliquity, SVAngle EcLong, SVAngle EcLat, SVAngle outRA, SVAngle outDec) Set the current (RA, Dec) coordinates of the SkyPoint, given pointers to its Ecliptic (Long, Lat) coordinates, and to the current obliquity angle (the angle between the equator and ecliptic).
static void	KSSkyPoint.nutate(KSNumbers num, SVAngle inRA, SVAngle inDec, SVAngle outRA, SVAngle outDec) Determine the effects of nutation for this SkyPoint.
static void	KSSkyPoint.aberrate(KSNumbers num, SVAngle inRA, SVAngle inDec, SVAngle outRA, SVAngle outDec, boolean addAbberation) Determine the effects of aberration for this SkyPoint.
static void	KSSkyPoint.precessFromAnyEpoch(double jd0, double jdf, SVAngle RA0, SVAngle Dec0, SVAngle RA, SVAngle Dec) General case of precession.
static SVRADec	KSSkyPoint.Eterms(SVAngle inRA, SVAngle inDec) Determine the E-terms of aberration In the past, the mean places of stars published in catalogs included the contribution to the aberration due to the ellipticity of the orbit of the Earth.
static void	KSSkyPoint.B1950ToJ2000(SVAngle RA, SVAngle Dec) Exact precession from Besselian epoch 1950 to epoch J2000.
static void	KSSkyPoint.J2000ToB1950(SVAngle RA, SVAngle Dec) Exact precession from epoch J2000 Besselian epoch 1950.
static void	KSSkyPoint.addEterms(SVAngle RA, SVAngle Dec) Coordinates in the FK4 catalog include the effect of aberration due to the ellipticity of the orbit of the Earth.
static void	KSSkyPoint.subtractEterms(SVAngle RA, SVAngle Dec) Coordinates in the FK4 catalog include the effect of aberration due to the ellipticity of the orbit of the Earth.
void	SVAngle.set(SVAngle d) Copy value of another dms angle
SVAngle	SVAngle.getReducedDiff(SVAngle rhs)
SVAngle	SVAngle.getDiff(SVAngle rhs)
static SVAzAlt	SVGeometry.EquatorialToHorizontal(SVAngle LST, SVAngle lat, SVAngle inRA, SVAngle inDec) Determine the (Altitude, Azimuth) coordinates of the SkyPoint from its (RA, Dec) coordinates, given the local sidereal time and the observer's latitude.
static SVRADec	SVGeometry.HorizontalToEquatorial(SVAngle LST, SVAngle lat, SVAngle az, SVAngle alt) Convert Horizontal coordinates (Azimuth, Altitude) to Equatorial coordinates (RA, Dec), given the local sidereal time and the observer's latitude.
static SVAngle	SVTime.getLocalSidrealTime(double julianDate, SVAngle longitude) TODO Make this compensate for nutation in longitude, the web page tells how to do this Note: Setting longitude to 0 (zero) will return greenwhich sidreal time http://aa.usno.navy.mil/faq/docs/GAST.html This is accurate to +/- 1.5 arcseconds

Constructors in edu.pdx.starview.calc with parameters of type SVAngle

KSSkyPoint(SVAngle r, SVAngle d)
Default constructor: Sets RA, Dec and RA0, Dec0 according to arguments.

SVAngle(SVAngle d)
Copy-Constructor

SVAzAlt(SVAngle az, SVAngle alt)
Constructor

SVRADec(SVAngle theRA, SVAngle theDec)
Constructor

Uses of SVAngle in edu.pdx.starview.data

Methods in edu.pdx.starview.data with parameters of type SVAngle

SVAzAlt

SVStar.getApparentAzAlt(SVTime theTime, SVAngle latitude, SVAngle longitude) Calculate apparent place of star For our telescope...

Constructors in edu.pdx.starview.data with parameters of type SVAngle

SVStar(SVAngle theRA_Cat, SVAngle theMu_RA, SVAngle theDec_Cat, SVAngle theMu_Dec, double theMag, java.lang.String theName, double CatEquinox, double CatEpoch)
Constructor

Uses of SVAngle in edu.pdx.starview.imaging

Methods in edu.pdx.starview.imaging with parameters of type SVAngle

static ImageMap	ImageGeneration.genImage(java.io.File SAO_Database, SVAngle lat, SVAngle longi, SVAngle azimuthCenter, SVAngle altitudeCenter, int imageWidth, int imageHeight, SVTime theTime, SVAngle arcWidthOfImage) Generates an image of the sky based on location, time and other specifications.
void	ImageMap.drawStar(SVAngle CurrentAz, SVAngle CurrentAlt) Deprecated.
void	ImageMap.drawStar(SVAngle objectAzIn, SVAngle objectAltIn, SVSkyObject objectInfo) Draws a point in the sky where a star or planet will be.
static java.util.Vector	SVFilter.starFilter(KSNumbers date, SVAngle lat, SVAngle lng, SVAngle az, SVAngle alt, double M_in, double N_in, double min_mag, double max_mag, java.util.Vector fullDB)

Constructors in edu.pdx.starview.imaging with parameters of type SVAngle

ImageMap(int w, int h, SVAngle CenterAz, SVAngle CenterAlt, SVAngle imageAngle)
Used to create images of the sky based on azimuth and altitude of the objects in the sky, and based on what direction your looking.

Uses of SVAngle in edu.pdx.starview.planets

Methods in edu.pdx.starview.planets with parameters of type SVAngle

static SVAzAlt	PlanetData.getAzAltOfPlanet(int thePlanet, double JDOfObservation, SVAngle observerLat, SVAngle observerLong)
static SVAzAlt[]	PlanetData.getAllPlanetLocs(double JDOfObservation, SVAngle observerLat, SVAngle observerLong)