Fig. 2 from A Model for Hard X‐Ray Emission from the Top of Flaring Loops

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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. 2.

Pitch‐angle distribution of electrons in the looptop region (x = 0–5 × 10⁸ cm, y = 1.3–1.8 × 10⁹ cm, at energies >30 keV [solid line] and >50 keV [dashed line]). The particle number is the time‐integrated number of test particles recorded in the simulation.

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