Estimation of Solar System acceleration from VLBI
Transactions of IAA RAS, issue 21, 240–242 (2010)
Keywords: радиоинтерферометрия со сверхдлинными базами, РСДБ-наблюдения, ускорение Солнечной системы, барицентр, вековая аберрация, программный пакет QUASAR, вектор ускорения
Abstract
The estimation of Solar System acceleration was obtained. Obtained value compared with the results of other authors. Calculation was performed by the global adjustment of the VLBI data using QUASAR software. The estimated value of acceleration a = (4.7 ± 0.5) × 10^-10 м/c2; α = 288° ± 5°; δ = 0° ± 5° - significantly differs from the theoretical one but comparable with the other results.
Citation
S. Kurdubov. Estimation of Solar System acceleration from VLBI // Transactions of IAA RAS. — 2010. — Issue 21. — P. 240–242.
@article{kurdubov2010,
abstract = {The estimation of Solar System acceleration was obtained. Obtained value compared with the results of other authors. Calculation was performed by the global adjustment of the VLBI data using QUASAR software. The estimated value of acceleration a = (4.7 ± 0.5) × 10^-10 м/c2; α = 288° ± 5°; δ = 0° ± 5° - significantly differs from the theoretical one but comparable with the other results.},
author = {S. Kurdubov},
issue = {21},
journal = {Transactions of IAA RAS},
keyword = {радиоинтерферометрия со сверхдлинными базами, РСДБ-наблюдения, ускорение Солнечной системы, барицентр, вековая аберрация, программный пакет QUASAR, вектор ускорения},
pages = {240--242},
title = {Estimation of Solar System acceleration from VLBI},
url = {http://iaaras.ru/en/library/paper/727/},
year = {2010}
}
TY - JOUR
TI - Estimation of Solar System acceleration from VLBI
AU - Kurdubov, S.
PY - 2010
T2 - Transactions of IAA RAS
IS - 21
SP - 240
AB - The estimation of Solar System acceleration was obtained. Obtained
value compared with the results of other authors. Calculation was
performed by the global adjustment of the VLBI data using QUASAR
software. The estimated value of acceleration a = (4.7 ± 0.5) ×
10^-10 м/c2; α = 288° ± 5°; δ = 0° ± 5° - significantly differs from
the theoretical one but comparable with the other results.
UR - http://iaaras.ru/en/library/paper/727/
ER -