Faraday Dispersion in the Solar Atmosphere.
نویسندگان
چکیده
منابع مشابه
The Solar Atmosphere
Looking at the solar photosphere, we see the top of the convection zone in the form of granulation: Hot gas rising from the solar interior as part of the energy transport process reaches a position where the opacity is no longer sufficient to prevent the escape of radiation. The gas expands, radiates, and cools and in so doing loses its buoyancy and descends. These motions, ultimately driven by...
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ژورنال
عنوان ژورنال: The Astronomical Journal
سال: 1960
ISSN: 0004-6256
DOI: 10.1086/108095