Solar Cycle Variation in Solar f-Mode Frequencies and Radius View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2000-03

AUTHORS

H.M. Antia, Sarbani Basu, J. Pintar, B. Pohl

ABSTRACT

Using data from the Global Oscillation Network Group (GONG) covering the period from 1995 to 1998, we study the change with solar activity in solar f-mode frequencies. The results are compared with similar changes detected from the Michelson Doppler Imager (MDI) data. We find variations in f-mode frequencies which are correlated with solar activity indices. If these changes are due to variation in solar radius then the implications are that the solar radius decreases by about 5 km from minimum to maximum activity. More... »

PAGES

459-468

Identifiers

URI

http://scigraph.springernature.com/pub.10.1023/a:1005204800696

DOI

http://dx.doi.org/10.1023/a:1005204800696

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1007081194


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