Detection of Solar Gravity Mode Oscillations,

Abstract

An analysis of solar velocity data obtained at the Stanford Solar Observatory shows the existence of solar global oscillations in the range 45 to 105 microHz (160 to 370 minutes). These oscillations are interpreted as internal gravity modes of degree l = 1 and l = 2. A good estimate of the order of the modes has also been made. (Author)

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Document Details

Document Type
Technical Report
Publication Date
Apr 01, 1983
Accession Number
ADA130289

Entities

People

  • Philip Scherrer
  • Philippe Delache

Organizations

  • Stanford University

Tags

Communities of Interest

  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Aeronautics
  • Atmospheric Sciences
  • Contracts
  • Crystal Lattice Vibrations
  • Data Reduction
  • Data Sets
  • Doppler Effect
  • Frequency
  • Identification
  • Military Research
  • Observation
  • Observatories
  • Oscillation
  • Power Spectra
  • Sidelobes
  • Solar Observatories
  • Spectra

Readers

  • Atmospheric Science / Meteorology, specifically Wind Wave Turbulence.
  • Solar Physics