Faraday rotation fluctuations of MESSENGER radio signals through the equatorial lower corona near solar minimum-Reference-Cited by-同舟云学术

Faraday rotation fluctuations of MESSENGER radio signals through the equatorial lower corona near solar minimum

Author:

Wexler D. B.¹,Jensen E. A.²,Hollweg J. V.³,Heiles C.⁴,Efimov A. I.⁵,Vierinen J.⁶⁷,Coster A. J.²^ORCID

Affiliation:

1. Computational Engineering and Science Research Centre; University of Southern Queensland; Toowoomba Australia

2. Planetary Science Institute; Tucson Arizona

3. Department of Physics; University of New Hampshire; Durham New Hampshire

4. Department of Astronomy; University of California; Berkeley Berkeley California

5. Kotel'nikov Institute of Radio Engineering and Electronics; Moscow Russia

6. Department of Physics and Technology; University of TromsØ; Tromsø Norway

7. MIT Haystack Observatory; Westford Massachusetts

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Link

Reference52 articles.

3. Wave heating of the solar atmosphere;Arregui;Phil. Trans. R. Soc. Ser. A,2015

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