This week the Sun featured a very long filament that stretched at least half way across the Sun (Oct. 20-22, 2015). Filaments are elongated clouds of plasma that are tethered above the Sun by magnetic forces. They are often unstable and usually break apart in less than a week, though they can last longer than that. Filaments are darker than most of the Sun surface when viewed in extreme ultraviolet light, as it is here.
I like astronomy, archaeology, photography, music and drinking a lot of tea. I hate politics. Something that annoys me: that I shall not respect the permanence, and to take me by what I'm not. The best sign: VIRGO. The worst: the health. The best: adapt and know how to get ahead. FIRST BLOG: esplaobs.blogspot.com, SECOND BLOG: esplaobs02.blogspot.com, RETRO BLOG: esplaobs01.blogspot.com, YOUTUBE CHANNELS: esplaobs, esplaobs. ext02. Instagram: esplaobsrosario. Welcome to my BLOGs !
Saturday, October 24, 2015
REALLY LONG FILAMENT Credit: Solar Dynamics Observatory, NASA.
This week the Sun featured a very long filament that stretched at least half way across the Sun (Oct. 20-22, 2015). Filaments are elongated clouds of plasma that are tethered above the Sun by magnetic forces. They are often unstable and usually break apart in less than a week, though they can last longer than that. Filaments are darker than most of the Sun surface when viewed in extreme ultraviolet light, as it is here.
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