Proxy Magnetometry of the Photosphere: Why are G-Band Bright Points so Bright?

Details Proxy Magnetometry of the Photosphere: Why are G-Band Bright Points so Bright? Proxy Magnetometry of the Photosphere: Why are G-Band Bright Points so Bright?

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aspc..236..445r&link_type=gif

Advanced Solar Polarimetry -- Theory, Observation, and Instrumentation -- 20TH NSO/Sac Summer Workshop, ASP Conference Proceedin

Astronomy and Astrophysics

Astronomy

26

Scientific paper

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