Regularized reconstruction of the differential emission measure from solar flare hard X-ray spectra

Prato, M., Piana, M., Brown, J.C., Emslie, A.G., Kontar, E.P. and Massone, A.M. (2006) Regularized reconstruction of the differential emission measure from solar flare hard X-ray spectra. Solar Physics, 237(1), pp. 61-83. (doi:10.1007/s11207-006-0029-1)

Full text not currently available from Enlighten.

Publisher's URL:


We address the problem of how to test whether an observed solar hard X-ray bremsstrahlung spectrum (<i>I</i>(∊)) is consistent with a purely thermal (locally Maxwellian) distribution of source electrons, and, if so, how to reconstruct the corresponding differential emission measure (ξ(<i>T</i>)). Unlike previous analysis based on the Kramers and Bethe-Heitler approximations to the bremsstrahlung cross-section, here we use an exact (solid-angle-averaged) cross-section. We show that the problem of determining ξ(<i>T</i>) from measurements of <i>I</i>(∊) involves two successive inverse problems: the first, to recover the mean source-electron flux spectrum (<i><div style="text-decoration: overline;">F</div></i>(<i>E</i>)) from <i>I</i>(∊) and the second, to recover ξ(T) from <i><div style="text-decoration: overline;">F</div></i>(<i>E</i>). We discuss the highly pathological numerical properties of this second problem within the framework of the regularization theory for linear inverse problems. In particular, we show that an iterative scheme with a positivity constraint is effective in recovering δ-like forms of ξ(<i>T</i>) while first-order Tikhonov regularization with boundary conditions works well in the case of power-law-like forms. Therefore, we introduce a restoration approach whereby the low-energy part of <i><div style="text-decoration: overline;">F</div></i>(<i>E</i>), dominated by the thermal component, is inverted by using the iterative algorithm with positivity, while the high-energy part, dominated by the power-law component, is inverted by using first-order regularization. This approach is first tested by using simulated <i><div style="text-decoration: overline;">F</div></i>(<i>E</i>) derived from a priori known forms of ξ(<i>T</i>) and then applied to hard X-ray spectral data from the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI).<i><div style="text-decoration: overline;">F</div></i>

Item Type:Articles
Glasgow Author(s) Enlighten ID:Kontar, Professor Eduard and Brown, Professor John and Piana, Professor Michele and Massone, Dr Anna
Authors: Prato, M., Piana, M., Brown, J.C., Emslie, A.G., Kontar, E.P., and Massone, A.M.
Subjects:Q Science > QB Astronomy
Q Science > QC Physics
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Solar Physics

University Staff: Request a correction | Enlighten Editors: Update this record