CORONAL ALFVÉN WAVES DETECTED BY RADIO SOUNDING DURING THE SOLAR OCCULTATIONS OF THE HELIOS SPACECRAFT

Author:

Bird M.K.,Volland H.,Efimov A.I.,Levy G.S.,Seidel B.L.,Stelzried C.T.

Publisher

Elsevier

Reference9 articles.

1. The temperature structure, mass and energy flow in the corona and inner solar wind;Withbroe;Ap.J.,1988

2. Large-scale structure of the interplanetary medium;Schwenn,1990

3. Possible evidence for coronal Alfvén waves;Hollweg;J. Geophys. Res.,1982

4. Remote sensing observations of the solar corona;Bird,1990

5. Solar wind motion within 30 R⊙: Spacecraft radio scintillation observations;Armstrong;Astron. Astrophys.,1981

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1. Multipoint radio probe of the solar corona: The trans-coronal radio array fleet;Frontiers in Astronomy and Space Sciences;2022-11-03

2. Modern Faraday Rotation Studies to Probe the Solar Wind;Frontiers in Astronomy and Space Sciences;2022-04-13

3. CORONAL FARADAY ROTATION FLUCTUATIONS AND A WAVE/TURBULENCE-DRIVEN MODEL OF THE SOLAR WIND;The Astrophysical Journal;2010-09-30

4. Coronal Faraday rotation of occulted radio signals;Astronomical & Astrophysical Transactions;2007-12

5. Kilometre-scale structures in the Sun's corona;Nature;1996-01

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