Determination of the line structure in solar p-mode frequency spectra. IPHIR data analysis

Astronomy and Astrophysics

Volumn 310, Issue 2, 1996, Pages 651-660

  Gavryusev, V G ^a,c   Gavryuseva, E A ^a,b  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b INSTITUTE FOR NUCLEAR RESEARCH   (Russian Federation)

^c MOSCOW STATE UNIVERSITY   (Russian Federation)

Author keywords

Methods: data analysis; Sun: oscillations; rotation

Indexed keywords

EID: 0000698755     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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