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Solar Flares
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Abstract
When we look at a solar flare we observe at relatively close hand a sample of the most energetic phenomena in the universe. These dynamic eruptions can only truly be appreciated from time-lapse movies or spectra. They fill the interplanetary medium with cosmic rays and shock waves, and produce plasmas with temperatures of 50 million degrees. They are rewarding both from the astrophysical and aesthetic points of view.
Additional Information
This work was supported by NASA under grant NGR 05 002 034 and NSF under grant Ga. 24015.Attached Files
Published - BBSO_#0111.pdf
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BBSO_#0111.pdf
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(17.5 MB)
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Additional details
Identifiers
- Eprint ID
- 34565
- Resolver ID
- CaltechAUTHORS:20120928-194739781
Funding
- NASA
- NGR 05 002 034
- NSF
- GA 24015
Dates
- Created
-
2012-10-04Created from EPrint's datestamp field
- Updated
-
2023-03-09Created from EPrint's last_modified field