args[0]=message
args[1]=DB::DB::Message=HASH(0x399fd40)
Re[3]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2
25.12.2008 11:06 | S. Yu. Yudin
Citata: |
pryamoe voshozhdenie i sklonenie dany topocentricheskie bez vsyakih redukcii. |
Zdravstvuite Vadim, bol'shoe spasibo. Vse Vashi soobsheniya yavlyayutsya dlya menya ochen' cennymi i topocentricheskoe predstavlenie dannyh mnogoe stanovit na svoi mesta, no s moimi fragmentarnymi poznaniyami v astronomii i v chastnosti po ustroistvu astronomicheskih instrumentov mne, vse taki, ne vse ponyatno i ya schitayu, chto v razdele Original Data dolzhny byli byt' dany dannye v gorizontal'noi sisteme koordinat. Hotya ya ne ponimayu, kak i v gorizontal'noi sisteme koordinat mogli byt' polucheny original'nye dannye meridiannyh nablyudenii v doteleskopicheskuyu eru. Ved' (kak ya ponimayu) meridiannye nablyudeniya proizvodyatsya v tot moment, kogda svetilo raspolozheno v meridiannom kruge, a Merkurii i Venera mogut tuda popast' tol'ko togda, kogda nedaleko ot nih nahoditsya Solnce i bez teleskopa ih nikak ne budet vidno. Daite pozhaluista poyasneniya a to mne nado budet obrabatyvat' eshe i dannye Ptolemeya, a menya glozhut vsyakie somneniya po povodu metodiki obrabotki ego dannyh. Ya, naprimer, podozrevayu, chto on nablyudal eti svetila v moment voshoda i zakata, a potom privodil eti koordinaty s uchetom popravki na vremya nablyudeniya k koordinatam, kotorye budut pri prohozhdenie etimi svetilami meridiana, a v takom sluchae refrakciya budet drugaya.
I eshe, Vadim poyasnite mne pozhaluista v formate dannyh Parizhskogo byuro dolgot smysl Coordinate Type. V dannyh, kotorye privodit Parizhskogo byuro dolgot pishetsya tol'ko App (smotrite prodolzhenie stroki dannyh, kotorye ya privodil v pervom soobshenie dlya Merkuriya ot 29 sentyabrya 1924 goda)
5 53 34.4000 1.0000 PARI various transits 0.0 Trans App
Eti dannye rasshifrovyvayutsya tak
dec. and
sigma A1, I2, 1X, I1, 1X, F7.4, 1X, F7.4, Deg Min ArcSec Sec 3X,
Observatory
A4, 1X,
Instrument A11, 1X,
Focal Length F5.1, in
cm. 2X,
Observation Type A5, (Trans)it, (Micro)meter, (Photo)
graphic, or CCD 2X,
Coordinate Type A5, (App)arent J2000, B1950, or other
epoch
Zdes' mne ne ponyatno App oznachaet, chto eto vidimye koordinaty dlya epohi i ravnodenstviya J2000 ili prosto vidimye koordinaty i dlya epohi B1950 dolzhno byt' napisano App B1950 ili prosto B1950. Sudya po formatu dannyh Pulkovskoi observatorii, poluchaetsya, chto prosto B1950, t.k. u nih napisano 1950.0, no hotelos' by eto utochnit'. Kstati, dal'she oni ukazyvayut v kakih koordinatah privedeny dannye t topocentricheskie i g - geocentricheskie i u nih byvaet dazhe, chto dlya odnoi planety oni idut vperemeshku i ne ponyatno, zachem oni odni dannye, poluchennye v topocentricheskoi sisteme, perevodyat v geocentricheskie, a drugie ne perevodyat. Vot primer Pulkovskih dannyh
1972 2 1.677390 23 21 57.770 -5.25061111 1950.0 t
A eshe v reducirovannyh dannyh Parizhskogo
byuro dolgot posle Coordinate Type idut i drugie parametry, rasshifrovki kotoryh v formate
dannyh net.
+20 17 22.0500 0.5500 84 Trans App True Geo FK4
Kak ya ponimayu, Geo oznachaet, chto eto geocentricheskie koordinaty, a FK4 eto nazvanie kataloga, no ya ne ponimayu, prichem zdes' katalog i chto znachit True, esli eti koordinaty dany dlya standartnoi epohi J2000.
S nailuchshimi pozhelaniyami Sergei Yudin.
- Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 17.12.2008 17:41, 18.9 KBait, otvetov: 17)
- Re: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 18.12.2008 11:20, 614 Bait, otvetov: 16)
- Re[2]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (V. V. Chazov, 24.12.2008 13:49, 171 Bait, otvetov: 15)
- >> Re[3]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 25.12.2008 11:06, 3.4 KBait, otvetov: 14)
- Re[4]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (V. V. Chazov, 25.12.2008 14:01, 1.5 KBait, otvetov: 12)
- Re[5]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 26.12.2008 23:27, 3.3 KBait, otvetov: 11)
- Re[6]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 4.03.2009 16:27, 14.3 KBait)
- Re[6]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 4.03.2009 16:32, 14.8 KBait, otvetov: 9)
- Re[7]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 27.04.2009 11:45, 12.0 KBait, otvetov: 8)
- Re[8]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 27.04.2009 11:47, 16.2 KBait, otvetov: 7)
- Re[9]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 29.04.2009 18:59, 3.8 KBait, otvetov: 6)
- Re[10]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 15.06.2009 9:53, 1.7 KBait, otvetov: 5)
- Re[11]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (Aleksei Dovgyallo, 4.03.2010 14:37, 239 Bait, otvetov: 4)
- Re[12]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (Aleksei Dovgyallo, 5.03.2010 13:20, 929 Bait, otvetov: 2)
- Re[13]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (P. V. Fedotov, 1.05.2010 7:46, 1.7 KBait, otvetov: 1)
- Re[14]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 15.01.2011 23:38, 2.6 KBait)
- Re[12]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (S. Yu. Yudin, 6.03.2010 23:29, 248 Bait)
- Re[4]: Metodika obrabotki dannyh astronomicheskih nablyudenii 2 (V. V. Chazov, 25.12.2008 14:05, 1.4 KBait)