z-logo
open-access-imgOpen Access
Data-driven Model of Temporal Evolution of Solar Mg ii h and k Profiles over the Solar Cycle
Author(s) -
J. Koza,
S. Gunár,
P. Schwartz,
P. Heinzel,
W.J. Liu
Publication year - 2022
Publication title -
the astrophysical journal supplement series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.546
H-Index - 277
eISSN - 1538-4365
pISSN - 0067-0049
DOI - 10.3847/1538-4365/ac69cf
Subject(s) - physics , astrophysics , solar prominence , radiative transfer , coronal mass ejection , solar flare , extreme ultraviolet , solar cycle 24 , solar cycle , atmospheric radiative transfer codes , flare , spectral line , k line , astronomy , plasma , solar wind , optics , stars , magnetic field , laser , quantum mechanics

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom