9780792322382 - Developments in Astrometry and Their Impact on Astrophysics and Geodynamics: Proceedings of the 156th Symposium of the International Astronomical . . ... Shanghai, ... (16 resultados)

Condición: New.

Condición: New.

Condición: As New. Unread book in perfect condition.

Condición: New. In.

Condición: New.

Condición: As New. Unread book in perfect condition.

Condición: New. Proceedings of the 156th Symposium of the International Astronomical Union, held in Shanghai, China, September 15-19, 1992 Editor(s): Mueller, Ivan I.; Kolaczek, Barbara (Space Research Centre, Polish Academy of Sciences, Warsaw, Poland). Series: International Astronomical Union Symposia (Closed). Num Pages: 440 pages, biography. BIC Classification: PG. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 24. Weight in Grams: 662. . 1993. Softcover reprint of the original 1st ed. 1993. Paperback. . . . .

Condición: New. pp. 476.

Taschenbuch. Condición: Neu. Developments in Astrometry and Their Impact on Astrophysics and Geodynamics | Proceedings of the 156th Symposium of the International Astronomical Union Held in Shanghai, China, September 15-19, 1992 | Ivan I. Mueller (u. a.) | Taschenbuch | XXXI | Englisch | 1993 | Springer | EAN 9780792322382 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Condición: New. Proceedings of the 156th Symposium of the International Astronomical Union, held in Shanghai, China, September 15-19, 1992 Editor(s): Mueller, Ivan I.; Kolaczek, Barbara (Space Research Centre, Polish Academy of Sciences, Warsaw, Poland). Series: International Astronomical Union Symposia (Closed). Num Pages: 440 pages, biography. BIC Classification: PG. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 24. Weight in Grams: 662. . 1993. Softcover reprint of the original 1st ed. 1993. Paperback. . . . . Books ship from the US and Ireland.

Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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.

Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 476 pp. Englisch.

Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the 156th Symposium of the International Astronomical Union, held in Shanghai, China, September 15-19, 1992 In this review talk, I would like to report on the proper motion analysis, which has been recently carried out together with .

Condición: New. Print on Demand pp. 476 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam.

Condición: New. PRINT ON DEMAND pp. 476.

Taschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -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.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 476 pp. Englisch.