Solar eclipses as an astrophysical laboratory

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作者
Jay M. Pasachoff
机构
[1] Williams College — Hopkins Observatory,Department of Planetary Sciences
[2] 33 Lab Campus Drive,undefined
[3] Williamstown,undefined
[4] Massachusetts 01267,undefined
[5] USA ,undefined
[6] California Institute of Technology 150-21,undefined
[7] Pasadena,undefined
[8] California 91125,undefined
[9] USA,undefined
来源
Nature | 2009年 / 459卷
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摘要
Astronomers no longer have to wait for a total solar eclipse before they can make meaningful observations of the Sun's corona. Earth- and satellite-based coronagraphs make such observations routine. But as Jay Pasachoff explains in a Review (one of a series commissioned for the International Year of Astronomy, collected on http://tinyurl.com/prhcqy), a new generation of eclipse studies is linking solar observations from satellites with ground-based observations in spatial, time and spectral-resolution domains that are inaccessible from space. Eventually, as space-based solar telescopes proliferate, they may take over completely from Earth-bound observation. But for the next 600 million years or so — until the Moon's distance from the Sun increases such that its disk becomes too small to block out the sunlight — the solar eclipse will remain one of the best shows on Earth.
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页码:789 / 795
页数:6
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