Mesogranulation in 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: Journal of Physical Studies
سال: 2012
ISSN: 1027-4642,2310-0052
DOI: 10.30970/jps.16.3902