The Solar Rotation Rate Ω(R, θ)

Details The Solar Rotation Rate Ω(R, θ) The Solar Rotation Rate Ω(R, θ)

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..347e&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 347-350 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

In recent years, the capability to detect and analyse solar oscillation
acoustic modes has greatly improved. The development of ground based
networks like GONG or BiSON and the use of space platforms like SOHO has
allowed us to study the structure and dynamics of the Sun with
unprecedented precision.

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