Radio Occultation Observations of the Solar Corona Over 1.60–1.86 R ⊙ : Faraday Rotation and Frequency Shift Analysis-Reference-Cited by-同舟云学术

Radio Occultation Observations of the Solar Corona Over 1.60–1.86 R ⊙ : Faraday Rotation and Frequency Shift Analysis

Published:2019-10 Issue:10 Volume:124 Page:7761-7777
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Wexler David. B.¹^ORCID,Hollweg Joseph V.²,Efimov Anatoli I.³^ORCID,Song Paul⁴,Jensen Elizabeth A.⁵^ORCID,Lionello Roberto⁶^ORCID,Vierinen Juha⁷^ORCID,Coster Anthea J.⁸^ORCID

Affiliation:

1. Centre for Astrophysics University of Southern Queensland Toowoomba Queensland Australia

2. Department of Physics University of New Hampshire Durham NH USA

3. Kotel'nikov Institute of Radio Engineering and Electronics, Fryazino Branch Russian Academy of Sciences Fryazino Russia

4. Department of Physics University of Massachusetts Lowell Lowell MA USA

5. Planetary Science Institute Tuscon AZ USA

6. Predictive Science, Inc. San Diego CA USA

7. Department of Physics and Technology University of Tromsø Tromsø Norway

8. MIT Haystack Observatory Westford MA USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA026937

Reference64 articles.

1. Slow Solar Wind: Observations and Modeling

2. Interpretation of Electron Densities from Corona Brightness

3. Properties of coronal Alfvén waves from polarized radio occulatation experiments

4. Wave heating of the solar atmosphere

5. Tempurature Tomography of the Soft X‐Ray Corona: Measurements of Electron Densities, Tempuratures, and Differential Emission Measure Distributions above the Limb

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