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A Model for Hard X‐Ray Emission from the Top of Flaring Loops

  • Authors: L. Fletcher and P. C. H. Martens

Fletcher & Martens 1998 The Astrophysical Journal 505 418.

  • Provider: AAS Journals

Caption: Fig. 3.

Pitch‐angle distribution of electrons in the looptop region, at energies >30 keV (solid line) and >50 keV (dashed line), normalized to the maximum number in each energy range. The dotted line is the isotropic [f(θ) = sin θ] distribution.

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