File:Full Sun.jpg: Difference between revisions
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imported>Hhudson (Simulated EOVSA full-day synthesis maps at two representative frequencies, 2.8 GHz (the frequency of the F10.7 index), and 5 GHz. Note that a few of the bright, compact, sunspot related sources at 2.8 GHz are not seen at 5 GHz, because their magnetic fiel) |
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Latest revision as of 14:36, 1 November 2024
Simulated EOVSA full-day synthesis maps at two representative frequencies, 2.8 GHz (the frequency of the F10.7 index), and 5 GHz. Note that a few of the bright, compact, sunspot related sources at 2.8 GHz are not seen at 5 GHz, because their magnetic field strength in the model is lower than for the others. Such full-disk images will be made daily at hundreds of frequencies, and will be used to produce the first daily coronal magnetic field maps.
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