Fig. 10 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

Fletcher & Martens 1998 The Astrophysical Journal 505 418.

Caption: Fig. 10.

Coulomb loss rate for a proton power‐law distribution, δ = 3, low‐energy cutoff at 0.5 MeV, in an ambient loop density of 3 × 10¹⁰ cm⁻³.