Developments in Astrometry and Their Impact on Astrophysics and Geodynamics
نام عام مواد
[Book]
ساير اطلاعات عنواني
Proceedings of the 156th Symposium of the International Astronomical Union Held in Shanghai, China, September 15-19, 1992 /
نام نخستين پديدآور
edited by Ivan I. Mueller, Barbara Kołaczek.
وضعیت نشر و پخش و غیره
محل نشرو پخش و غیره
Dordrecht :
نام ناشر، پخش کننده و غيره
Imprint: Springer,
تاریخ نشرو بخش و غیره
1993.
فروست
عنوان فروست
International Astronomical Union / Union Astronomique Internationale ;
مشخصه جلد
156
یادداشتهای مربوط به مندرجات
متن يادداشت
Space Optical Astrometry -- Ground-Based Optical Astrometry -- Very Long Baseline Interferometry (VLBI) -- Impact on Astrophysics -- Impact on Geodynamics -- Celestial Reference Frame -- Terrestrial Reference Frame -- Miscellaneous -- Author Index.
بدون عنوان
0
یادداشتهای مربوط به خلاصه یا چکیده
متن يادداشت
In this review talk, I would like to report on the proper motion analysis, which has been recently carried out together with M. Soma and M. Yoshizawa: There has been a persistent demand in astronomy for accurate stellar positions and proper motions, which are represented by an inertial reference system constructed on the basis of a set of consistent astronomical constants. In the reference system the precessional constant plays a primary role. In a series of papers Fricke (1967a,b, 1977a,b) has deter mined the luni-solar precessional correction to Newcomb's value and the fictitious motion of the equinox, which have been adopted in the "IAU (1976) System of Astronomical Con stants". Based on the precessional correction and the equinoctial motion thus established, the fundamental reference system, the FK5 system (Fricke et al. 1988) for positions and proper motions, has been constructed. However, for several years geodetic VLBI (McCarthy & Luzum 1991) and LLR (Williams et at. 1991) observations have been suggesting an additional correction to the luni-solar precessional constant of the IAU (1976) System. That is, these observations indicate the precessional correction of 6. p ~ -0:'30/cent to the FK5 system. But, the observational period ofthe earth orientation is considered to be still insufficient to separate unambiguously the precessional change of the earth orientation from the nutation with the longest period of 18. 6 years.
ویراست دیگر از اثر در قالب دیگر رسانه
شماره استاندارد بين المللي کتاب و موسيقي
9780792322382
قطعه
عنوان
Springer eBooks
عنوان اصلی به زبان دیگر
عنوان اصلي به زبان ديگر
Proceedings of the 156th Symposium of the International Astronomical Union, held in Shanghai, China, September 15-19, 1992
موضوع (اسم عام یاعبارت اسمی عام)
موضوع مستند نشده
Physical geography.
موضوع مستند نشده
Physics.
نام شخص به منزله سر شناسه - (مسئولیت معنوی درجه اول )