Particle and magnetic field properties of the Saturnian magnetosheath: Presence and upstream escape of hot magnetospheric plasma-Reference-Cited by-同舟云学术

Particle and magnetic field properties of the Saturnian magnetosheath: Presence and upstream escape of hot magnetospheric plasma

Author:

Sergis N.¹,Jackman C. M.²³,Masters A.⁴,Krimigis S. M.¹⁵,Thomsen M. F.⁶,Hamilton D. C.⁷,Mitchell D. G.⁵,Dougherty M. K.⁸,Coates A. J.⁹¹⁰

Affiliation:

1. Office of Space Research and Technology; Academy of Athens; Athens Greece

2. Department of Physics and Astronomy; University College London; London UK

3. Centre for Planetary Sciences; UCL/Birkbeck; London UK

4. Institute of Space and Astronautical Science; JAXA; Sagamihara Kanagawa Japan

5. The Johns Hopkins University; Applied Physics Laboratory; Laurel Maryland USA

6. Los Alamos National Laboratory; Los Alamos New Mexico USA

7. Department of Physics; University of Maryland; College Park Maryland USA

8. Space and Atmospheric Physics Group, The Blackett Laboratory; Imperial College London; London UK

9. Mullard Space Science Laboratory, Department of Space and Climate Physics; University College London; Surrey UK

10. The Centre for Planetary Sciences at UCL/Birkbeck; London UK

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

Reference38 articles.

3. Upstream of Saturn and Titan;Arridge;Space Sci. Rev.,2011

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