A comparison between photospheric and chromospheric quiet-Sun magnetograms

Details A comparison between photospheric and chromospheric quiet-Sun magnetograms A comparison between photospheric and chromospheric quiet-Sun magnetograms

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..194...19z&link_type=abstract

Solar Physics, v. 194, Issue 1, p. 19-28 (2000).

Physics

9

Scientific paper

Photospheric (Fei λ5324.19 Å line) and chromospheric (Hβ line) magnetic fields in quiet-Sun regions have been observed in the solar disk center by using the vector video magnetograph at Huairou Solar Observing Station of Beijing Astronomical Observatory. Observational results show that the quiet-Sun magnetic elements in the solar photosphere and chromosphere present similar magnetic structures. Photospheric and chromospheric magnetograms show corresponding time variations. This suggests that the magnetic fields in quiet-Sun regions present different 3-D magnetic configurations compared to those in solar active regions.

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