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Titlebook: Astronomy on the Personal Computer; Oliver Montenbruck,Thomas Pfleger Textbook 19983rd edition Springer-Verlag Berlin Heidelberg 1998 Ephe

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期刊全稱Astronomy on the Personal Computer
影響因子2023Oliver Montenbruck,Thomas Pfleger
視頻videohttp://file.papertrans.cn/164/163651/163651.mp4
發(fā)行地址Covers many topics of interest to the practical observer.Provides practical solutions to a variety of astronomical problems.Programs now run under Windows.Diskette contains the stars of the Zodiacal C
圖書封面Titlebook: Astronomy on the Personal Computer;  Oliver Montenbruck,Thomas Pfleger Textbook 19983rd edition Springer-Verlag Berlin Heidelberg 1998 Ephe
影響因子It is said that a typical astronomer of the 19th century spent seven hours working at a desk for every hour spent at the telescope. That‘s how long the routine analysis of data took with pencil, paper, and logarithmic tables. Thus when Wilhelm Olbers discovered the minor planet Vesta in 1807 and gathered the necessary observations, his friend Gauss needed almost 10 hours to hand- calculate its orbit. That achievement astonished many less gifted astronomers of the time, who might have labored days to work out the orbit of a newfound comet. How different things are today! Gauss‘s method of orbit determination, presented in Chap. 11 of this book, runs to completion on a home computer in a few seconds at most. The machine will issue its accurate results in less time than it takes to key in the observations. In this book, a landmark in the youthful literature of astronomical com- puter algorithms, Oliver Montenbruck and Thomas Pfleger cover many topics of keen interest to the practical observer. For me its most remarkable feature is the library of interrelated program modules, all elegantly written in PAS- CAL. Anyone who has tried to create such modules in interpreted BASIC soon runs i
Pindex Textbook 19983rd edition
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https://doi.org/10.1007/978-3-662-28729-3Moon, and then reappears on the other side after a certain interval. In total, there are about one thousand stars visible to the naked eye that the Moon may occult. They lie in a narrow band to the north and south of the ecliptic, and are never more than 8° distant from it.
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Stellar Occultations,Moon, and then reappears on the other side after a certain interval. In total, there are about one thousand stars visible to the naked eye that the Moon may occult. They lie in a narrow band to the north and south of the ecliptic, and are never more than 8° distant from it.
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https://doi.org/10.1007/978-3-662-32987-0rvations must be available..Bucerius’ method of orbit determination described here, is mainly derived from that of Gauss, but certain points have been considerably simplified. There are some restrictions on its use, therefore, but it is easier to understand and to employ.
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