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Nonthermal emission theory, modeling and inversions

Nonthermal emission theory, modeling and inversions. Gregory D. Fleishman. ?. Almost No SXRs!. 24 October 2001. AR 9672. NoRH images. 1. 2. 3. 4. 17 GHz I. 17 GHz V. 34 GHz I. Uniform, optically thin source with strong Razin-effect. Simplfied model fitting

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Nonthermal emission theory, modeling and inversions

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  1. Nonthermal emission theory, modeling and inversions Gregory D. Fleishman ?

  2. Almost No SXRs! 24 October 2001 AR 9672

  3. NoRH images 1 2 3 4 17 GHz I 17 GHz V 34 GHz I

  4. Uniform, optically thin source with strong Razin-effect Simplfied model fitting Sequence of fitted spectra Derived parameters vs time

  5. Coherent Radio Burst

  6. Conclusions • Theory and interpretation of nonthermal electromagnetic emission from astrophysical objects suggest a lot of new interesting physical studies. • Many specific problems within this field are well suited for undergraduate and graduate research projects and will substantially improve understanding of what we really see in astrophysical observations.

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