Solar cycle variations in p-modes and chromospheric magnetism

Details Solar cycle variations in p-modes and chromospheric magnetism Solar cycle variations in p-modes and chromospheric magnetism

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..152..261j&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 152, no. 1, p. 261-266

Physics

20

Chromosphere, Magnetic Effects, P Waves, Solar Cycles, Variability, Frequency Shift, Magnetic Field Configurations, Solar Activity, Stellar Models, Temperature Distribution

Scientific paper

The effect on p-mode frequencies of a horizontal chromospheric canopy field is studied theoretically and the results compared with Libbrecht and Woodard's observations of frequency changes. Combined changes in field strength and chromospheric temperature cause frequency shifts that are similar in form to those observed. Frequency shifts in p-modes offer the possibility of signatures of solar activity cycles distinct from sunspot numbers and butterfly diagrams.

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