X-RAY SOURCE HEIGHTS IN A SOLAR FLARE: THICK-TARGET VERSUS THERMAL CONDUCTION FRONT HEATING
Authors: J. W. Reep, S. J. Bradshaw, and G. D. Holman
2016 The Astrophysical Journal81844.
Provider: AAS Journals
Caption: Figure 3.
Source heights calculated for the thermal models, Runs 13–24, from left to right and from top to bottom. The timings, depths, and dispersion by energy are all inconsistent with the observed trends.