1. Comparison of 30 THz impulsive burst time development to microwaves, H-alpha, EUV, and GOES soft X-rays
- Author
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Miteva, R., Kaufmann, P., Cabezas, D. P., Cassiano, M. M., Fernandes, L. O. T., Freeland, S. L., Karlicky, M., Kerdraon, A., Kudaka, A. S., Luoni, M. L., Marcon, R., Raulin, J. -P., Trottet, G., and White, S. M.
- Subjects
Astrophysics - Solar and Stellar Astrophysics - Abstract
The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretation challenges. One event associated with a GOES M2 class flare has been observed simultaneously in microwaves, H-alpha, EUV, and soft X-ray bands. Although these new observations confirm some features found in the two prior known events, they exhibit time profile structure discrepancies between 30 THz, microwaves, and hard X-rays (as inferred from the Neupert effect). These results suggest a more complex relationship between 30 THz emission and radiation produced at other wavelength ranges. The multiple frequency emissions in the impulsive phase are likely to be produced at a common flaring site lower in the chromosphere. The 30 THz burst emission may be either part of a nonthermal radiation mechanism or due to the rapid thermal response to a beam of high-energy particles bombarding the dense solar atmosphere., Comment: accepted to Astronomy and Astrophysics
- Published
- 2015
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