Plasma Parameters From Quasi‐Thermal Noise Observed by Parker Solar Probe: A New Model for the Antenna Response

Author:

Martinović Mihailo M.12ORCID,Ðorđević Antonije R.34,Klein Kristopher G.1ORCID,Maksimović Milan2,Issautier Karine2ORCID,Liu Mingzhe2,Pulupa Marc5ORCID,Bale Stuart D.5678ORCID,Halekas Jasper S.9ORCID,McManus Michael D.5

Affiliation:

1. Lunar and Planetary Laboratory University of Arizona Tucson AZ USA

2. LESIA Observatoire de Paris Université PSL CNRS Sorbonne Université Université de Paris Meudon France

3. School of Electrical Engineering University of Belgrade Belgrade Serbia

4. Serbian Academy of Sciences and Arts Belgrade Serbia

5. Space Sciences Laboratory University of California Berkeley CA USA

6. School of Physics and Astronomy Queen Mary University of London London UK

7. Physics Department University of California Berkeley CA USA

8. The Blackett Laboratory Imperial College London London UK

9. Department of Physics and Astronomy University of Iowa Iowa IA USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference53 articles.

1. Импеданс и шумы антенны (зонда) в космической плаз мы;Andronov A. A.;Космические исследования,1966

2. Highly structured slow solar wind emerging from an equatorial coronal hole

3. The FIELDS Instrument Suite for Solar Probe Plus

4. Coronal Electron Temperature Inferred from the Strahl Electrons in the Inner Heliosphere: Parker Solar Probe and Helios Observations

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