Zobrazeno 1 - 10
of 11
pro vyhledávání: '"C. Y. Hohenkerk"'
Publikováno v:
Proceedings of the International Astronomical Union. 14:160-162
Analysis of historical records of eclipses of the Sun and Moon between 720 BC and AD 1600 gives a measure of the time difference, TT − UT = ΔT. The first derivative in time along a smooth curve fitted to the values of Δ T measures the changes in
Publikováno v:
Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences. 477:20200776
Historical reports of solar eclipses are added to our previous dataset (Stephenson et al. 2016 Proc. R. Soc. A 472 , 20160404 ( doi:10.1098/rspa.2016.0404 )) in order to refine our determination of centennial and longer-term changes since 720 BC in t
This material consists of the tables of the observational data prior to 1600, discussion of the comparative accuracy of Babylonian time intervals, a commentary on critical eclipses and a list of rejected observations. Lastly, a table of coefficients
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd4aa2135abde101f294b460df598610
Autor:
C Y Hohenkerk, J L Hilton
Publikováno v:
Metrologia. 48:S195-S199
An astronomical or navigational almanac can best be thought of as a device for connecting an observer with celestial objects. For an observer with a known position and time the almanac allows the observer to identify the celestial objects. Conversely
Autor:
C. Y. Hohenkerk, J. L. Hilton
Publikováno v:
Astronomy & Astrophysics. 413:765-770
Recommendation VII of Resolution A4 of the XXIst General Assembly of the International Astronomical Union (IAU 1992) states, in part, "... that the principal plane of the new conventional celestial reference system be as near as possible to the mean
Publikováno v:
Proceedings. Mathematical, Physical, and Engineering Sciences
New compilations of records of ancient and medieval eclipses in the period 720 BC to AD 1600, and of lunar occultations of stars in AD 1600–2015, are analysed to investigate variations in the Earth’s rate of rotation. It is found that the rate of
Autor:
E. M. Standish, J. Chapront, V. K. Abalakin, J.-E. Arlot, T. Fukushima, M.-F. He, C. Y. Hohenkerk, G. H. Kaplan, H. Kinoshita, G. A. Krasinsky, J. H. Lieske, H. Schwan, P. K. Seidelmann
Publikováno v:
Transactions of the International Astronomical Union. 24:7-10
The Commission has established its own website (http://ssd.jpl.nasa.gov/iau-comm4/) containing the following main topics: InformationWhere to Obtain EphemeridesRecent Papers and Information Related to EphemeridesObservational Data(Measurements to whi
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 238:1529-1535
Une equation qui donne l'equation du temps comme fonction du temps universel est developpee
Autor:
B. D. Yallop, C. Y. Hohenkerk
Publikováno v:
Solar Physics. 68:303-305
A diagram of the distribution in latitude of sunspot groups during the period 1874–1976 is given. As an indication of sunspot activity, a diagram of the mean total daily sunspot areas for each synodic rotation is also given.
Publikováno v:
The Astronomical Journal. 97:265