Variation of VIRGO/SOHO measurements during 1996-2001

Details Variation of VIRGO/SOHO measurements during 1996-2001 Variation of VIRGO/SOHO measurements during 1996-2001

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517..413v&link_type=abstract

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,

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Solar Irradiance

Scientific paper

Here, the correlation analysis of VIRGO/SOHO measurements of total solar irradiance during 1996-2001 has been carried out. The correlograms of 1996 and 1998 show that there is clear and strong evidence of solar rotational modulation. The rotational modulation is more in 1998 than that in 1996, however, the data of 1998 shows a splitting in the modulation peak. The synodic rotation period is estimated to be about 27 days. The variation of rotational modulation is independent of solar activity and it is found to be drastically different than other solar emission e.g. solar Lyman-Alpha, radio emission etc. There exists a large yearly variation in the correlograms having periodic and aperiodic peaks.

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