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A Spectral Analysis of the Masuda Flare Using Yohkoh Hard X‐Ray Telescope Pixon Reconstruction

  • Authors: David Alexander and Thomas R. Metcalf

Alexander & Metcalf 1997 The Astrophysical Journal 489 442.

  • Provider: AAS Journals

Caption: Fig. 1.

Comparison of pixon and MEM calculations for the LO and M1 channels. Reconstructed HXT images for the LO and M1 channels produced with pixons are shown in (a) and (b), while the corresponding MEM maps are shown in (c) and (d). Each image is independently scaled, with the maximum value indicated on the figures. The images are negatives with solar north up and solar east to the left. The images are 64 × 64 pixels with a 2﹩\farcs﹩5 pixel size.

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