Two Unusual Episodes of ≈13-Day Variations II. Implications for the Solar Radio Flux Density, F10.7 cm

Details Two Unusual Episodes of ≈13-Day Variations II. Implications for the Solar Radio Flux Density, F10.7 cm Two Unusual Episodes of ≈13-Day Variations II. Implications for the Solar Radio Flux Density, F10.7 cm

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005soph..229..127c&link_type=abstract

Solar Physics, Volume 229, Issue 1, pp.127-133

Physics

Scientific paper

Additional analysis of the behavior of the international sunspot number (R) series and the solar radio flux density (F10.7 cm) series during two long (250 500 days) and distinct episodes of persistent ≈13-day variations (Crane, Solar Phys. 1998, 253, 177) is reported. The conclusion is that while the center-to-limb behavior of R does not change between solar minimum and solar maximum, F10.7 cm exhibits significantly less limb brightening at solar maximum than at solar minimum.

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