C. Frohlich et al., FIRST RESULTS FROM VIRGO, THE EXPERIMENT FOR HELIOSEISMOLOGY AND SOLAR IRRADIANCE MONITORING ON SOHO, Solar physics, 170(1), 1997, pp. 1-25
First results from the VIRGO experiment (Variability of solar IRradian
ce and Gravity Oscillations) on the ESA/NASA Mission SOHO (Solar and H
eliospheric Observatory) are reported. The observations started mid-Ja
nuary 1996 for the radiometers and sunphotometers and near the end of
March for the luminosity oscillation imager. The performance of all th
e instruments is very good, and the time series of the first 4-6 month
s are evaluated in terms of solar irradiance variability, solar backgr
ound noise characteristics and p-mode oscillations. The solar irradian
ce is modulated by the passage of active regions across the disk, but
not all of the modulation is straightforwardly explained in terms of s
unspot flux blocking and facular enhancement. Helioseismic inversions
of the observed p-mode frequencies are more-or-less in agreement with
the latest standard solar models. The comparison of VIRGO results with
earlier ones shows evidence that magnetic activity plays a significan
t role in the dynamics of the oscillations beyond its modulation of th
e resonant frequencies. Moreover, by comparing the amplitudes of diffe
rent components of p-mode multiplets, each of which are influenced dif
ferently by spatial inhomogeneity, we have found that activity enhance
s excitation.