Understanding Cassini RPWS Antenna Signals Triggered by Dust Impacts-Reference-Cited by-同舟云学术

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Understanding Cassini RPWS Antenna Signals Triggered by Dust Impacts

Published:2019-10-22 Issue:20 Volume:46 Page:10941-10950
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Ye S.‐Y.¹²^ORCID,Vaverka J.³,Nouzak L.³^ORCID,Sternovsky Z.⁴,Zaslavsky A.⁵,Pavlu J.³^ORCID,Mann I.⁶^ORCID,Hsu H.‐W.⁴^ORCID,Averkamp T. F.²^ORCID,Sulaiman A. H.²^ORCID,Pisa D.⁷^ORCID,Hospodarsky G. B.²^ORCID,Kurth W. S.²^ORCID,Horanyi M.⁴

Affiliation:

1. Department of Earth and Space Sciences Southern University of Science and Technology (SUSTech) Shenzhen China

2. Department of Physics and Astronomy The University of Iowa Iowa City IA USA

3. Faculty of Mathematics and Physics Charles University Prague Czechia

4. LASP University of Colorado Boulder Boulder CO USA

5. Observatoire de Paris Meudon France

6. Department of Physics and Technology The Arctic University of Norway Tromso Norway

7. Department of Space Physics IAP CAS Prague Czechia

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019GL084150

Reference71 articles.

1. Shot noise from grain and particle impacts in Saturn's ring plane

2. Partitioning of energy in hypervelocity impact against loose sand targets

3. Detection of electromagnetic pulses produced by hypervelocity micro particle impact plasmas

4. Characteristic temperatures of hypervelocity dust impact plasmas

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