Английская Википедия:Coronal rain

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Версия от 18:15, 21 февраля 2024; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} {{Short description|Plasma falling to the Sun's photosphere}} thumb|300px|A movie of the coronal rain (right limb of sun) in the 304 Å [[wavelength. The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. SDO collected one frame every 12 seconds so each second in this video corresponds to 6 mi...»)
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Шаблон:Short description

Файл:Coronal Rain.ogv
A movie of the coronal rain (right limb of sun) in the 304 Å wavelength. The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. SDO collected one frame every 12 seconds so each second in this video corresponds to 6 minutes of real time. The video covers 4:30 UTC on July 19th to 2:00 UTC on July 20th, a period of 21 hours and 30 minutes.

Coronal rain is a phenomenon that occurs in the Sun's corona when hot plasma cools and condenses in strong magnetic fields and falls to the photosphere. It is usually associated with active regions.[1][2][3][4][5][6]

References

Шаблон:Reflist

External links


Шаблон:Sun-stub