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
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201935285
Publication URI: http://dx.doi.org/10.1051/0004-6361/201935285
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics