Visibility of nonradial pulsation modes in solar continuum intensity measurements

Details Visibility of nonradial pulsation modes in solar continuum intensity measurements Visibility of nonradial pulsation modes in solar continuum intensity measurements

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..241t&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 241-246 (SEE N89-25819 19-92)

Computer Science

Numerical Analysis

8

Helioseismology, Solar Flux Density, Solar Oscillations, Solar Physics, Sun, Numerical Analysis, Opacity, Plancks Constant

Scientific paper

A calculation of the continuum emission integrated over the solar disk, and of its perturbations arising from different nonradial pulsation modes, is presented. In addition to geometrical effects (variations of the emitting areas) and Planck function variations, the influence of opacity changes in H- (the principal absorber at the wavelengths under consideration) is examined. The computations are carried out numerically for 500 and 826 nanometers, which correspond to different channels of the IPHIR/PHOBOS experiment. The relative importance of these different processes of flux modulation is discussed as a function of oscillation period and modal type.

Affiliated with

Also associated with

No associations

Rating

Visibility of nonradial pulsation modes in solar continuum intensity measurements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Visibility of nonradial pulsation modes in solar continuum intensity measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Visibility of nonradial pulsation modes in solar continuum intensity measurements will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1756017