Observations of solar p-modes with L of not greater than 5

Details Observations of solar p-modes with L of not greater than 5 Observations of solar p-modes with L of not greater than 5

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...216..253p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 216, no. 1-2, June 1989, p. 253-258. Research supported by CAICYT.

Astronomy and Astrophysics

Astrophysics

15

Helioseismology, P Waves, Radial Velocity, Solar Oscillations, Astronomical Spectroscopy, Stellar Spectrophotometry, Zeeman Effect

Scientific paper

Results are presented for the sun's radial velocity in integrated sunlight. A resonant scattering spectrometer has been used to determine the frequencies and amplitudes of p-modes with spherical harmonics of degree (l) of less than 3, and a second spectrophotometer, which observes part of the sun by means of a spatial filter, has been used to measure the frequencies and amplitudes of p-modes with l of not greater than 5. The frequencies at both ends of the p-mode 5-minute oscillations with l of between 3 and 5, inclusively, are obtained with greater precision than previous determinations.

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