Hot flow anomaly observed at Jupiter's bow shock

doi:10.1002/2017GL073175

GSTDTAP > 气候变化

DOI	10.1002/2017GL073175
	Hot flow anomaly observed at Jupiter's bow shock
	Valek, P. W.1,2; Thomsen, M. F.3; Allegrini, F.1,2; Bagenal, F.4; Bolton, S.1; Connerney, J.5; Ebert, R. W.1; Gladstone, R.1,2; Kurth, W. S.6; Levin, S.7; Louarn, P.8; Mauk, B.9; McComas, D. J.1,10,11; Pollock, C.12; Reno, M.1,13; Szalay, J. R.1; Weidner, S.11; Wilson, R. J.4
	2017-08-28
发表期刊	GEOPHYSICAL RESEARCH LETTERS
ISSN	0094-8276
EISSN	1944-8007
出版年	2017
卷号	44 期号:16
文章类型	Article
语种	英语
国家	USA; France
英文摘要	A Hot Flow Anomaly (HFA) is created when an interplanetary current sheet interacts with a planetary bow shock. Previous studies have reported observing HFAs at Earth, Mercury, Venus, Mars, and Saturn. During Juno's approach to Jupiter, a number of its instruments operated in the solar wind. Prior to crossing into Jupiter's magnetosphere, Juno observed an HFA at Jupiter for the first time. This Jovian HFA shares most of the characteristics of HFAs seen at other planets. The notable exception is that the Jovian HFA is significantly larger than any HFA seen before. With an apparent size greater than 2x10(6)km the Jovian HFA is orders of magnitude larger than those seen at the other planets. By comparing the size of the HFAs at the other planets with the Jovian HFA, we conclude that HFAs size scales with the size of planetary bow shocks that the interplanetary current sheet interacts with.
英文关键词	Hot flow anomaly Jupiter Bow shock Juno
领域	气候变化
收录类别	SCI-E
WOS记录号	WOS:000410658800002
WOS关键词	DIAMAGNETIC CAVITIES UPSTREAM ; SOLAR-WIND ; DAWN FLANK ; MAGNETOSPHERE ; MAGNETOPAUSE ; SPACECRAFT
WOS类目	Geosciences, Multidisciplinary
WOS研究方向	Geology
引用统计
文献类型	期刊论文
条目标识符	http://119.78.100.173/C666/handle/2XK7JSWQ/26488
专题	气候变化
作者单位	1.Southwest Res Inst, Space Sci & Engn Div, San Antonio, TX 78238 USA; 2.Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA; 3.Planetary Sci Inst, Tucson, AZ USA; 4.Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA; 5.Goddard Space Flight Ctr, Greenbelt, MD USA; 6.Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA; 7.Jet Prop Lab, Pasadena, CA USA; 8.Univ Toulouse, CNRS, IRAP, UPS, Toulouse, France; 9.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA; 10.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA; 11.Princeton Univ, Princeton Plasma Phys Lab, Off Vice President, POB 451, Princeton, NJ 08543 USA; 12.Denali Sci, Healy, AK USA; 13.Austin Mission Consulting, Austin, TX USA
推荐引用方式 GB/T 7714	Valek, P. W.,Thomsen, M. F.,Allegrini, F.,et al. Hot flow anomaly observed at Jupiter's bow shock[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(16).
APA	Valek, P. W..,Thomsen, M. F..,Allegrini, F..,Bagenal, F..,Bolton, S..,...&Wilson, R. J..(2017).Hot flow anomaly observed at Jupiter's bow shock.GEOPHYSICAL RESEARCH LETTERS,44(16).
MLA	Valek, P. W.,et al."Hot flow anomaly observed at Jupiter's bow shock".GEOPHYSICAL RESEARCH LETTERS 44.16(2017).