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Publikováno v:
Geophysical Research Letters. 46:14282-14289
Autor:
J. Mukherjee, Steven J. Schwartz, Christopher T. Russell, S. A. Fuselier, James L. Burch, H. R. Lai, M. J. Starkey, M. I. Desai, R. G. Gomez
Publikováno v:
Geophysical Research Letters. 46:10735-10743
Autor:
Xianzhe Jia, Yingdong Jia, Christopher T. Russell, Jun Cui, H. R. Lai, Michele K. Dougherty, Adam Masters
In steady state, magnetic flux conservation must be maintained in Saturn’s magnetosphere. The Enceladus plumes add mass to magnetic flux tubes in the inner magnetosphere, and centrifugal force pulls the mass-loaded flux tubes outward. Those flux tu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bcee98da8877a15f60ed74164341e8b5
http://hdl.handle.net/10044/1/92720
http://hdl.handle.net/10044/1/92720
Publikováno v:
Geophysical Research Letters. 48
Publikováno v:
Earth and Planetary Physics.
Solar Wind (SW) electron precipitation is able to deposit a substantial amount of energy in the nightside Martian upper atmosphere, potentially exerting an influence on its thermal structure. This study serves as the first investigation of such an is
The phenomenon, dubbed the Interplanetary Field Enhancement, occurs in the solar wind near and inside of 1 AU and is attributed to collisional dust production and subsequent solar wind pickup. The duration and strength of these events appears to depe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fda40a5024ffb0f49271d7aad982b8d0
https://doi.org/10.5194/epsc2020-44
https://doi.org/10.5194/epsc2020-44
Publikováno v:
Journal of Geophysical Research: Space Physics. 125
Autor:
Yong Wei, Jun Cui, Zhipeng Ren, H. R. Lai, Xueke Wu, M.‐H. Fu, Junjian Guo, Zhaopeng Wu, H. Gu
Publikováno v:
Geophysical Research Letters. 47
As an important species of the Martian thermosphere, NO is chemically and radiatively active. However, its abundance is poorly constrained due to difficulties in both remote sensing and in situ measurements. In this study, we use the Neutral Gas and
Interplanetary Field Enhancements are phenomena in the interplanetary magnetic field, first discovered near Venus, during an extremely long duration (12 hours) and large size (about 0.1 AU) passage across the Pioneer Venus spacecraft. Three and a hal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::830537a99388a78162611c89f7271961
https://doi.org/10.5194/egusphere-egu2020-2476
https://doi.org/10.5194/egusphere-egu2020-2476