2D non-LTE modelling of a filament observed in the H a line with the DST/IBIS spectropolarimeter (2019)
Attributed to:
Understanding how solar eruptions begin and evolve through the solar atmosphere
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201935358
Publication URI: http://dx.doi.org/10.1051/0004-6361/201935358
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics