Обложка Solar Rotation
Название книги:

Solar Rotation

Betascript Publishing (2010-07-27 )

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ISBN-13:

978-613-1-05884-4

ISBN-10:
6131058849
EAN:
9786131058844
Язык Книги:
Английский
Краткое описание:
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Solar rotation is able to vary with latitude because the Sun is composed of a gaseous plasma. The rate of rotation is observed to be fastest at the equator (latitude φ=0 deg), and to decrease as latitude increases. At the equator the solar rotation period is 24.47 days. This is called the sidereal rotation period, and should not be confused with the synodic rotation period of 26.24 days, which is the time for a fixed feature on the Sun to rotate to the same apparent position as viewed from Earth. The synodic period is longer because the Sun must rotate for a sidereal period plus an extra amount due to the orbital motion of the Earth around the Sun.
Издательский Дом:
Betascript Publishing
Веб-сайт:
https://www.betascript-publishing.com/
Edited by:
Lambert M. Surhone, Miriam T. Timpledon, Susan F. Marseken
Количество страниц:
100
Опубликовано:
2010-07-27
Акции:
В наличии
Категория:
Физика, астрономия
Цена:
34.00 €
Ключевые слова:
Plasma, Differential Rotation, Sidereal, Synodic

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