Mars plasma system response to solar wind disturbances during solar minimum-Reference-Cited by-同舟云学术

Mars plasma system response to solar wind disturbances during solar minimum

Published:2017-06 Issue:6 Volume:122 Page:6611-6634
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Sánchez‐Cano B.¹^ORCID,Hall B. E. S.¹^ORCID,Lester M.¹^ORCID,Mays M. L.²^ORCID,Witasse O.³^ORCID,Ambrosi R.⁴,Andrews D.⁵^ORCID,Cartacci M.⁶,Cicchetti A.⁶^ORCID,Holmström M.⁷,Imber S.¹^ORCID,Kajdič P.⁸,Milan S. E.¹^ORCID,Noschese R.⁶,Odstrcil D.⁹,Opgenoorth H.⁵^ORCID,Plaut J.¹⁰,Ramstad R.⁷^ORCID,Reyes‐Ayala K. I.⁸

Affiliation:

1. Radio and Space Plasma Physics Group, Department of Physics and AstronomyUniversity of Leicester Leicester UK

2. Heliophysics Science DivisionNASA Goddard Space Flight Center Greenbelt Maryland USA

3. European Space AgencyESTEC‐Scientific Support Office Noordwijk Netherlands

4. Space Research Centre, Department of Physics and AstronomyUniversity of Leicester Leicester UK

5. Swedish Institute of Space Physics Uppsala Sweden

6. Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica Rome Italy

7. Swedish Institute of Space Physics Kiruna Sweden

8. Instituto de GeofísicaUniversidad Nacional Autónoma de México, Ciudad Universitaria Mexico City Mexico

9. School of Physics, Astronomy, and Computational SciencesGeorge Mason University Fairfax Virginia USA

10. Jet Propulsion Laboratory Pasadena California USA

Funder

Science and Technology Facilities Council

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA023587

Reference81 articles.

1. Magnetic Field and Plasma Observations at Mars: Initial Results of the Mars Global Surveyor Mission

2. Global Distribution of Crustal Magnetization Discovered by the Mars Global Surveyor MAG/ER Experiment

3. Dayside induced magnetic field in the ionosphere of Mars

4. Geoeffectiveness of corotating interaction regions as measured byDstindex

5. Determination of local plasma densities with the MARSIS radar: Asymmetries in the high-altitude Martian ionosphere

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