Signatures of the non-Maxwellian $?$-distributions in optically thin line spectra. II. Synthetic Fe XVII--XVIII X-ray coronal spectra and predictions for the Marshall Grazing-Incidence X-ray Spectrometer (MaGIXS) (2019)
Attributed to:
UNDERSTANDING THE DYNAMICAL SOLAR ATMOSPHERE
funded by
STFC
Abstract
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Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1905.10356
Publication URI: https://arxiv.org/abs/1905.10356
Type: Other