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High-density O+ in Earth's outer magnetosphere and its effect on dayside magnetopause magnetic reconnection
Alternative TitleWOS:000504368100001
Fuselier, S. A.; Mukherjee, J.; Denton, M. H.; Petrinec, S. M.; Trattner, K. J.; Toledo-Redondo, S.; Andre, M.; Aunai, N.; Chappell, C. R.; Glocer, A.; Haaland, S.; Hesse, M.; Kistler, L. M.; Lavraud, B.; Li, W. Y.; Moore, T. E.; Graham, D.; Tenfjord, P.; Dargent, J.; Vines, S. K.; Strangeway, R. J.; Burch, J. L.
Source PublicationJOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
2019
Volume124Issue:12Pages:10257-10269
DOI10.1029/2019JA027396
ISSN2169-9380
Language英语
KeywordMagnetospheric plasma composition Magnetopause Magnetic reconnection Solar Wind-Magnetosphere interaction-
AbstractThe warm plasma cloak is a source of magnetospheric plasma that contain significant O+. When the O+ density in the magnetosphere near the magnetopause is >0.2 cm(-3) and the H+ density is <1.5 cm(-3), then O+ dominates the magnetospheric ion mass density by more than a factor of 2. A survey is conducted of such O+-rich warm plasma cloak intervals and their effect on reconnection at the Earth's magnetopause. The survey uses data from the Magnetospheric Multiscale mission (MMS) and the results are compared and combined with a previous survey of the warm plasma cloak. Overall, the warm plasma cloak and the O+-rich warm plasma cloak reduce the magnetopause reconnection rate by >20% due to mass-loading only about 2% to 4% of the time. However, during geomagnetic storms, O+ dominates the mass density of the warm plasma cloak and these mass densities are very high. Therefore, a separate study is conducted to determine the effect of the warm plasma cloak on magnetopause reconnection during geomagnetically disturbed times. This study shows that the warm plasma cloak reduces the reconnection rate significantly about 25% of the time during disturbed conditions.
Indexed BySCI
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Cited Times:3[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/7559
Collection中国科学院国家空间科学中心
Affiliation1.[Fuselier, S. A.
2.Mukherjee, J.
3.Burch, J. L.] Southwest Res Inst, San Antonio, TX 78238 USA
4.[Fuselier, S. A.] Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
5.[Denton, M. H.] New Mexico Consortium, Los Alamos, NM USA
6.[Petrinec, S. M.] Lockheed Martin Adv Technol Ctr, Palo Alto, CA USA
7.[Trattner, K. J.] Univ Colorado, Atmospher & Space Phys Lab, Campus Box 392, Boulder, CO 80309 USA
8.[Toledo-Redondo, S.
9.Lavraud, B.] Univ Toulouse, Inst Rech Astrophys & Planetol, CNRS, UPS,CNES, Toulouse, France
10.[Andre, M.
11.Graham, D.] Swedish Inst Space Phys, Uppsala, Sweden
12.[Aunai, N.] Lab Phys Plasmas, Palaiseau, France
13.[Chappell, C. R.] Vanderbilt Univ, 221 Kirkland Hall, Nashville, TN 37235 USA
14.[Glocer, A.
15.Moore, T. E.] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
16.[Haaland, S.] Max Planck Inst, Katlenburg Lindau, Germany
17.[Hesse, M.
18.Tenfjord, P.] Univ Bergen, Bergen, Norway
19.[Kistler, L. M.] Univ New Hampshire, Durham, NH 03824 USA
20.[Li, W. Y.] Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China
21.[Dargent, J.] Univ Pisa, Phys Dept E Fermi, Pisa, Italy
22.[Vines, S. K.] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
23.[Strangeway, R. J.] Univ Calif Los Angeles, Earth & Space Sci, Los Angeles, CA USA
Recommended Citation
GB/T 7714
Fuselier, S. A.,Mukherjee, J.,Denton, M. H.,et al. High-density O+ in Earth's outer magnetosphere and its effect on dayside magnetopause magnetic reconnection[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2019,124(12):10257-10269.
APA Fuselier, S. A..,Mukherjee, J..,Denton, M. H..,Petrinec, S. M..,Trattner, K. J..,...&Burch, J. L..(2019).High-density O+ in Earth's outer magnetosphere and its effect on dayside magnetopause magnetic reconnection.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,124(12),10257-10269.
MLA Fuselier, S. A.,et al."High-density O+ in Earth's outer magnetosphere and its effect on dayside magnetopause magnetic reconnection".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 124.12(2019):10257-10269.
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