现在的位置:主页 > 期刊导读 >

行星低频射电爆发的空间探测进展(10)

来源:北极光 【在线投稿】 栏目:期刊导读 时间:2021-05-22

【作者】网站采编

【关键词】

【摘要】[25]DOUGHERTY M K,CAO H,KHURANA K K,et al. Saturn's magnetic field revealed by the Cassini Grand Finale[J]. Science,2018,362(6410):46. [26]LELLOUCH E,MCGRATH M E,JESSUP K L. Io's a

[25]DOUGHERTY M K,CAO H,KHURANA K K,et al. Saturn's magnetic field revealed by the Cassini Grand Finale[J]. Science,2018,362(6410):46.

[26]LELLOUCH E,MCGRATH M E,JESSUP K L. Io's atmosphere[M]//Io After Galileo :a New View of Jupiter’s Volcanic Moon. [S. l.]:Springer Praxis Publishing Ltd,2007:231-264.

[27]ZARKA P,FARGES T,RYABOV B P,et al. A scenario for Jovian S-bursts[J]. Geophysical Research Letters,1996,23(2):125-128.

[28]LADREITER H P,ZARKA P,LECACHEUX A. Direction-finding study of Jovian hectometric and broadband kilometric radio emissions:Evidence for their auroral origin[J]. Planetary and Space,1994,42:919-931.

[29]KIMURA T,TSUCHIYA F,MISAWA H,et al. Radiation characteristics of quasi-periodic radio bursts in the Jovian high-latitude region[J]. Planetary and Space Science,2008,56(15):1967-1976.

[30]MORIOKA A,NOZAWA H,MISAWA H,et al. ,Rotationally driven quasi-periodic radio emissions in the Jovian magnetosphere[J]. Journal of Geophysical Research,2006,111:A04223.

[31]BHATTACHARYA A B,RAHA B. Detection of radio emissions from Jupiter[J]. OJP,2013,5(1-2):1-12.

[32]GURNETT D A,KURTH W S,HOSPODARSKY G B,et ak. Control of Jupiter's radio emission and aurorae by the solar wind[J]. Nature,2002,415:985-987.

[33]HOSPODARSKY G B,KURTH W S,CECCONI B,et observations of Jovian quasi-periodic radio emissions by the Galileo and Cassini spacecraft[J]. Journal of Geophysical Research,2004,109:A09S07.

[34]BROWN S,JANSSEN M,ADUMITROAIE V,et al. ,Prevalent lightning sferics at 600 megahertz near Jupiter's poles[J]. Nature,2018,558:87-90.

[35]HIGGINS C A,CARR T D,REYES F. A new determination of Jupiter's radio rotation period[M]//Planetary Radio Emissions :Austrian Acad. Sci. Press,1997:43-50.

[36]WINTERHALTER D,KUIPER T,MAJID W,et al. Search for radio emissions from extrasolar planets:the observation campaign[M]//Planetary Radio Emissions VI. Vienna:Austrian Academy of Sciences Press,2006.

[37]ZARKA P. The search for exoplanetary radio emissions,in Planetary Radio Emissions VⅡ[M].Vienna:Austrian Academy of Sciences Press,2011:287-301.

[38]SIROTHIA S K,DES ETANGS A L,KRISHNA G,et al. Search for 150 MHz radio emission from extrasolar planets in the TIFR GMRT Sky Survey[J]. A&A,2014,562(2):A108.

[39]SHIMWELL T W,HAVERKORN M,CSEH D,et al. The LOFAR two-metre sky survey:I. survey description and preliminary data release[J]. Astronomy & Astrophysics,2017,598:A104.

[40]DES ETANGS A L,SIROTHIA S K,KRISHNA G,et al. Hint of 150 MHz radio emission from the Neptune-mass extrasolar transiting planet HAT-P-11b[J]. Astronomy & Astrophysics,2013,552:A65.

[41]VEDANTHAM H K,CALLINGHAM J R,SHIMWELL T W,et radio emission from a quiescent red dwarf indicative of star–planet interaction[J]. Nature Astronomy,2020,4:577-583.

[42]薛长斌,周晴,王雷,等. “嫦娥4号”任务有效载荷系统设计与实现[J]. 深空探测学报(中英文),2017,4(6): C B,ZHOU Q,WANG L,et al. Design and implementation of payload system in Chang’e–4 mission[J]. Journal of Deep Space Exploration,2017,4(6):515-521.

[43]贾瑛卓,邹永廖,薛长斌,等. 嫦娥四号任务科学目标和有效载荷配置[J]. 空间科学学报,2018,38(1): Y Z,ZOU Y L,XUE C B,et al. Scientific objectives and payloads of Chang’ E-4 mission[J]. Chinese Journal of Space Science,2018,38(1):118-130.

文章来源:《北极光》 网址: http://www.bjgzzs.cn/qikandaodu/2021/0522/743.html

上一篇:唯美极光
下一篇:夜空中的色彩从何而来

北极光投稿 | 北极光编辑部| 北极光版面费 | 北极光论文发表 | 北极光最新目录
Copyright © 2018 《北极光》杂志社 版权所有
投稿电话: 投稿邮箱: