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Searched refs:longitude (Results 1 - 18 of 18) sorted by relevance

/third_party/icu/icu4c/source/i18n/
H A Dastro.h66 * The longitude specifies the position along the ecliptic plane
84 * @param lon The ecliptic longitude, measured in radians.
89 longitude = lon; in Ecliptic()
95 * @param lon The ecliptic longitude, measured in radians.
100 longitude = lon; in set()
118 * The ecliptic longitude, in radians.
128 double longitude; member in CalendarAstronomer::Ecliptic
274 * it takes for the moon to return the same ecliptic longitude as the sun.
275 * It is longer than the sidereal month because the sun's longitude increases
305 * latitude and longitude
[all...]
H A Dastro.cpp96 * it takes for the moon to return the same ecliptic longitude as the sun.
97 * It is longer than the sidereal month because the sun's longitude increases
109 * for the moon to return to the same ecliptic longitude relative to the
261 * latitude and longitude. The object's time is set to the current
264 * @param longitude The desired longitude, in <em>degrees</em> east of
274 CalendarAstronomer::CalendarAstronomer(double longitude, double latitude) : in CalendarAstronomer() argument
276 fLongitude = normPI(longitude * (double)DEG_RAD); in CalendarAstronomer()
448 return eclipticToEquatorial(result, ecliptic.longitude, ecliptic.latitude); in eclipticToEquatorial()
454 * @param eclipLong The ecliptic longitude
638 getSunLongitude(double jDay, double &longitude, double &meanAnomaly) getSunLongitude() argument
[all...]
/third_party/node/deps/icu-small/source/i18n/
H A Dastro.h66 * The longitude specifies the position along the ecliptic plane
84 * @param lon The ecliptic longitude, measured in radians.
89 longitude = lon; in Ecliptic()
95 * @param lon The ecliptic longitude, measured in radians.
100 longitude = lon; in set()
118 * The ecliptic longitude, in radians.
128 double longitude; member in CalendarAstronomer::Ecliptic
274 * it takes for the moon to return the same ecliptic longitude as the sun.
275 * It is longer than the sidereal month because the sun's longitude increases
305 * latitude and longitude
[all...]
H A Dastro.cpp96 * it takes for the moon to return the same ecliptic longitude as the sun.
97 * It is longer than the sidereal month because the sun's longitude increases
109 * for the moon to return to the same ecliptic longitude relative to the
261 * latitude and longitude. The object's time is set to the current
264 * @param longitude The desired longitude, in <em>degrees</em> east of
274 CalendarAstronomer::CalendarAstronomer(double longitude, double latitude) : in CalendarAstronomer() argument
276 fLongitude = normPI(longitude * (double)DEG_RAD); in CalendarAstronomer()
448 return eclipticToEquatorial(result, ecliptic.longitude, ecliptic.latitude); in eclipticToEquatorial()
454 * @param eclipLong The ecliptic longitude
638 getSunLongitude(double jDay, double &longitude, double &meanAnomaly) getSunLongitude() argument
[all...]
/third_party/skia/third_party/externals/icu/source/i18n/
H A Dastro.h66 * The longitude specifies the position along the ecliptic plane
84 * @param lon The ecliptic longitude, measured in radians.
89 longitude = lon; in Ecliptic()
95 * @param lon The ecliptic longitude, measured in radians.
100 longitude = lon; in set()
118 * The ecliptic longitude, in radians.
128 double longitude; member in CalendarAstronomer::Ecliptic
274 * it takes for the moon to return the same ecliptic longitude as the sun.
275 * It is longer than the sidereal month because the sun's longitude increases
305 * latitude and longitude
[all...]
H A Dastro.cpp96 * it takes for the moon to return the same ecliptic longitude as the sun.
97 * It is longer than the sidereal month because the sun's longitude increases
109 * for the moon to return to the same ecliptic longitude relative to the
261 * latitude and longitude. The object's time is set to the current
264 * @param longitude The desired longitude, in <em>degrees</em> east of
274 CalendarAstronomer::CalendarAstronomer(double longitude, double latitude) : in CalendarAstronomer() argument
276 fLongitude = normPI(longitude * (double)DEG_RAD); in CalendarAstronomer()
448 return eclipticToEquatorial(result, ecliptic.longitude, ecliptic.latitude); in eclipticToEquatorial()
454 * @param eclipLong The ecliptic longitude
638 getSunLongitude(double jDay, double &longitude, double &meanAnomaly) getSunLongitude() argument
[all...]
/third_party/python/Lib/
H A Dantigravity.py7 def geohash(latitude, longitude, datedow):
17 print('%d%s %d%s' % (latitude, p[1:], longitude, q[1:]))
/third_party/icu/icu4j/main/classes/core/src/com/ibm/icu/impl/
H A DCalendarAstronomer.java71 * it takes for the moon to return the same ecliptic longitude as the sun.
72 * It is longer than the sidereal month because the sun's longitude increases
83 * for the moon to return to the same ecliptic longitude relative to the
229 * latitude and longitude. The object's time is set to the current
232 * @param longitude The desired longitude, in <em>degrees</em> east of
241 public CalendarAstronomer(double longitude, double latitude) { in CalendarAstronomer() argument
243 fLongitude = normPI(longitude * DEG_RAD); in CalendarAstronomer()
428 return eclipticToEquatorial(ecliptic.longitude, ecliptic.latitude); in eclipticToEquatorial()
434 * @param eclipLong The ecliptic longitude
1537 public final double longitude; global() field in CalendarAstronomer.Ecliptic
[all...]
/third_party/icu/ohos_icu4j/src/main/java/ohos/global/icu/impl/
H A DCalendarAstronomer.java73 * it takes for the moon to return the same ecliptic longitude as the sun.
74 * It is longer than the sidereal month because the sun's longitude increases
85 * for the moon to return to the same ecliptic longitude relative to the
231 * latitude and longitude. The object's time is set to the current
234 * @param longitude The desired longitude, in <em>degrees</em> east of
243 public CalendarAstronomer(double longitude, double latitude) { in CalendarAstronomer() argument
245 fLongitude = normPI(longitude * DEG_RAD); in CalendarAstronomer()
430 return eclipticToEquatorial(ecliptic.longitude, ecliptic.latitude); in eclipticToEquatorial()
436 * @param eclipLong The ecliptic longitude
1540 public final double longitude; global() field in CalendarAstronomer.Ecliptic
[all...]
/third_party/icu/ohos_icu4j/src/main/tests/ohos/global/icu/dev/test/calendar/
H A DAstroTest.java43 // year, month, day, hour, minute, longitude (radians), ascension(radians), declination(radians) in TestSolarLongitude()
55 double longitude = astro.getSunLongitude(); in TestSolarLongitude()
56 if (longitude != tests[i][5]) { in TestSolarLongitude()
57 if ((float)longitude == (float)tests[i][5]) { in TestSolarLongitude()
58 logln("longitude(" + longitude + in TestSolarLongitude()
62 errln("FAIL: longitude(" + longitude + in TestSolarLongitude()
/third_party/icu/icu4j/main/tests/core/src/com/ibm/icu/dev/test/calendar/
H A DAstroTest.java40 // year, month, day, hour, minute, longitude (radians), ascension(radians), declination(radians) in TestSolarLongitude()
52 double longitude = astro.getSunLongitude(); in TestSolarLongitude()
53 if (longitude != tests[i][5]) { in TestSolarLongitude()
54 if ((float)longitude == (float)tests[i][5]) { in TestSolarLongitude()
55 logln("longitude(" + longitude + in TestSolarLongitude()
59 errln("FAIL: longitude(" + longitude + in TestSolarLongitude()
/third_party/skia/third_party/externals/piex/src/
H A Dpiex_types.h72 Rational longitude[3]; member
H A Dtiff_parser.cc92 preview_image_data->gps.longitude)) { in FillGpsPreviewImageData()
/third_party/icu/icu4c/source/test/intltest/
H A Dastrotst.cpp102 double longitude = astro->getSunLongitude(); in TestSolarLongitude() local
103 //longitude = 0; in TestSolarLongitude()
106 logln((UnicodeString)"Sun position is " + result.toString() + (UnicodeString)"; " /* + result.toHmsString()*/ + " Sun longitude is " + longitude ); in TestSolarLongitude()
/third_party/musl/Benchmark/musl/
H A Dlibc_stdio.cpp805 double longitude; in Bm_function_Sscanf_double() local
808 benchmark::DoNotOptimize(sscanf("113.123456789 31.123456789", "%lf %lf", &longitude, &latitude)); in Bm_function_Sscanf_double()
/third_party/ffmpeg/libavformat/
H A Dmovenc.c4166 double latitude, longitude, altitude; local
4176 longitude = strtod(ptr, &end);
4194 longitude_fix = (int32_t) ((1 << 16) * longitude);
4223 float latitude, longitude, altitude; local
4232 longitude = strtof(ptr, &end);
4247 longitudex10000 = (int32_t) (10000 * longitude);
4251 av_log(s, AV_LOG_WARNING, "longitude or latitude is not in range\n");
4272 // calc longitude
H A Dmov.c240 double longitude, latitude, altitude; in mov_metadata_loci() local
266 longitude = ((int32_t) avio_rb32(pb)) / (float) (1 << 16); in mov_metadata_loci()
271 snprintf(buf, sizeof(buf), "%+08.4f%+09.4f", latitude, longitude); in mov_metadata_loci()
/third_party/skia/third_party/externals/sfntly/java/lib/
H A Dicu4j-4_8_1_1.jar ... lang.Object { public final double latitude public final double longitude public void <init> (double, double) double lat double lon public ...

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