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X
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Above left, our galaxy in X-rays, above, a supernova
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Specs
1.54m focal length provides images from the .25 to 4.5 keV on a 1024x1024 cdc detector
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http://www.sciamarchive.org/qpdf.cfm?ArticleID_CHAR=275CD5E3-0A46-47CE-85FE-83E874D98BB
Yohkoh X-Ray Pictures
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The Corona
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Caused by strong magnetic fields that may span up to 500,000 square kilometers
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“An "arcade" is a system of magnetic loops organized into an elongated cylindrical formation. Often such an arcade will result from a slowly-developing solar flare or a coronal mass ejection (or both). The bright arcade may persist for days or longer.”
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These occur anywhere on the Sun at opposition of the active regions.
Caused by magnetic fields that are sucked down into the photosphere
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unipolar magnetic fields
high-speed solar wind streams originate in coronal holes
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large-scale magnetic loops connect two active regions
"emerging flux": magnetic loops push their way through the photosphere and appear in the corona
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The result of two opposed arcades resulting in explosions of x-rays from the sun
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The MAXIM
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