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authortpearson <tpearson@283d02a7-25f6-0310-bc7c-ecb5cbfe19da>2011-08-10 22:19:39 +0000
committertpearson <tpearson@283d02a7-25f6-0310-bc7c-ecb5cbfe19da>2011-08-10 22:19:39 +0000
commit49f9b290287ed4df63901c5912ddbb3c1ae5d515 (patch)
tree0a20bf2186d58b5edef3a3a7da518ea3c8244246 /kworldwatch/astro.c
parent1d14c95a7737078a695e99442628f450354c00ff (diff)
downloadtdetoys-49f9b290287ed4df63901c5912ddbb3c1ae5d515.tar.gz
tdetoys-49f9b290287ed4df63901c5912ddbb3c1ae5d515.zip
rename the following methods:
tqparent parent tqmask mask git-svn-id: svn://anonsvn.kde.org/home/kde/branches/trinity/kdetoys@1246260 283d02a7-25f6-0310-bc7c-ecb5cbfe19da
Diffstat (limited to 'kworldwatch/astro.c')
-rw-r--r--kworldwatch/astro.c14
1 files changed, 7 insertions, 7 deletions
diff --git a/kworldwatch/astro.c b/kworldwatch/astro.c
index 5d09dcd..3423119 100644
--- a/kworldwatch/astro.c
+++ b/kworldwatch/astro.c
@@ -7,7 +7,7 @@
long jdate(struct tm *);
double jtime(struct tm *);
double kepler(double m, double ecc);
-void sunpos(double jd, int aptqparent, double *ra, double *dec, double *rv, double *slong);
+void sunpos(double jd, int apparent, double *ra, double *dec, double *rv, double *slong);
double gmst(double jd);
/* JDATE -- Convert internal GMT date and time to Julian day
@@ -65,19 +65,19 @@ double m, ecc;
/* SUNPOS -- Calculate position of the Sun. JD is the Julian date
of the instant for which the position is desired and
- APPARENT should be nonzero if the aptqparent position
+ APPARENT should be nonzero if the apparent position
(corrected for nutation and aberration) is desired.
The Sun's co-ordinates are returned in RA and DEC,
both specified in degrees (divide RA by 15 to obtain
hours). The radius vector to the Sun in astronomical
units is returned in RV and the Sun's longitude (true
- or aptqparent, as desired) is returned as degrees in
+ or apparent, as desired) is returned as degrees in
SLONG. */
void
-sunpos(jd, aptqparent, ra, dec, rv, slong)
+sunpos(jd, apparent, ra, dec, rv, slong)
double jd;
-int aptqparent;
+int apparent;
double *ra, *dec, *rv, *slong;
{
double t, t2, t3, l, m, e, ea, v, theta, omega,
@@ -119,9 +119,9 @@ double *ra, *dec, *rv, *slong;
eps = 23.452294 - 0.0130125 * t - 0.00000164 * t2 + 0.000000503 * t3;
- /* Corrections for Sun's aptqparent longitude, if desired. */
+ /* Corrections for Sun's apparent longitude, if desired. */
- if (aptqparent) {
+ if (apparent) {
omega = fixangle(259.18 - 1934.142 * t);
theta = theta - 0.00569 - 0.00479 * sin(dtr(omega));
eps += 0.00256 * cos(dtr(omega));