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Прохождения Меркурия по диску Солнца (наблюдения 1631–1878 гг.)

Transactions of IAA RAS, issue 4, 69–79 (1999)

Keywords: радиоинтерферометрия со сверхдлинными базами (РСДБ), астрометрия, геодинамика, небесная механика, прохождения планет по диску Солнца, геометрическая интерпретация условий для наблюдений, механизм формирования изображения, явление "черной капли", визуальные наблюдения планеты вблизи края Солнца, задачи эфемеридной астрономии

Abstract

The geometrical interpretation of the conditions of observations is given for the transits of planets through the solar disk. The mechanism of the formation of Mercury's image and the “black drop” phenomenon are described for visual observations of planet near the limb of the Sun. The main problems of the ephemeris astronomy solved by observations of the transits are discussed briefly. The structure of archive of observations of transits, that created at IAA RAS, is described. The preliminary values of corrections $\Delta T^s$ to the scale $UT$ obtained by averaging (O−C) for moments of contacts at 1631–1878 are in good agreement with the results of Stephenson and Morrison.

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M. Sveshnikov. Прохождения Меркурия по диску Солнца (наблюдения 1631–1878 гг.) // Transactions of IAA RAS. — 1999. — Issue 4. — P. 69–79.

@article{sveshnikov1999,
  abstract = {The geometrical interpretation of the conditions of observations is given for the transits of planets through the solar disk. The mechanism of the formation of Mercury's image and the “black drop” phenomenon are described for visual observations of planet near the limb of the Sun. The main problems of the ephemeris astronomy solved by observations of the transits are discussed briefly. The structure of archive of observations of transits, that created at IAA RAS, is described. The preliminary values of corrections $\Delta T^s$ to the scale $UT$ obtained by averaging (O−C) for moments of contacts at 1631–1878 are in good agreement with the results of Stephenson and Morrison.},
  author = {M. Sveshnikov},
  issue = {4},
  journal = {Transactions of IAA RAS},
  keyword = {радиоинтерферометрия со сверхдлинными базами (РСДБ), астрометрия, геодинамика, небесная механика, прохождения планет по диску Солнца, геометрическая интерпретация условий для наблюдений, механизм формирования изображения, явление "черной капли", визуальные наблюдения планеты вблизи края Солнца, задачи эфемеридной астрономии},
  note = {russian},
  pages = {69--79},
  title = {Прохождения Меркурия по диску Солнца (наблюдения 1631–1878 гг.)},
  url = {http://iaaras.ru/en/library/paper/231/},
  year = {1999}
}

TY  - JOUR
TI  - Прохождения Меркурия по диску Солнца (наблюдения 1631–1878 гг.)
AU  - Sveshnikov, M.
PY  - 1999
T2  - Transactions of IAA RAS
IS  - 4
SP  - 69
AB  - The geometrical interpretation of the conditions of observations is
given for the transits of planets through the solar disk. The
mechanism of the formation of Mercury's image and the “black drop”
phenomenon are described for visual observations of planet near the
limb of the Sun. The main problems of the ephemeris astronomy solved
by observations of the transits are discussed briefly. The structure
of archive of observations of transits, that created at IAA RAS, is
described. The preliminary values of corrections $\Delta T^s$ to the
scale $UT$ obtained by averaging (O−C) for moments of contacts at
1631–1878 are in good agreement with the results of Stephenson and
Morrison.
UR  - http://iaaras.ru/en/library/paper/231/
ER  -