Origin of Certain Solar Emission Lines Between 170 and 220 Å.

Details Origin of Certain Solar Emission Lines Between 170 and 220 Å. Origin of Certain Solar Emission Lines Between 170 and 220 Å.

Jul 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964apj...140..390e&link_type=gif

Astrophysical Journal, vol. 140, p.390

Astronomy and Astrophysics

Astrophysics

15

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