Explanation: Recorded on July 7, this animation using X-ray images of the Sun shows an amazing event - three nearly simultaneous jets connected with solar active regions. The two frames were taken several hours apart by the Soft X-ray Telescope on board the orbiting Yohkoh observatory. They have a "negative" color scheme, the darker colors representing more intense X-rays from the corona and active regions on the solar surface. The pictures clearly show two curving jets of X-ray hot plasma appearing above the solar equator and one below. A sharp vertical stripe near the jet above center is a digital blemish while the overall shift of the image is due to solar rotation. As the Sun is now approaching the active part of its 11 year cycle, similar single jets are seen every week or so. But the appearance of these three widely separated jets at once is considered an unlikely coincidence and is fueling current speculations about their origins.
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
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Публикации с ключевыми словами:
Sun - active region - рентгеновское излучение - Солнце - Солнечная корона - космические обсерватории - джет
Публикации со словами: Sun - active region - рентгеновское излучение - Солнце - Солнечная корона - космические обсерватории - джет | |
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