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020 ▼a 9780438125353
035 ▼a (MiAaPQ)AAI10902928
035 ▼a (MiAaPQ)umichrackham:001191
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 247004
0820 ▼a 550
1001 ▼a Johnson, Blake C.
24510 ▼a Mars' Energetic Plume Ion Escape Channel.
260 ▼a [S.l.]: ▼b University of Michigan., ▼c 2018.
260 1 ▼a Ann Arbor: ▼b ProQuest Dissertations & Theses, ▼c 2018.
300 ▼a 160 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
500 ▼a Adviser: Michael Warren Liemohn.
5021 ▼a Thesis (Ph.D.)--University of Michigan, 2018.
520 ▼a Mars is losing its atmosphere. The planet's small size results in relatively low energy requirements for atmospheric particles to escape into deep space, and its lack of a planetary magnetic field allows the solar wind to directly interact with
590 ▼a School code: 0127.
650 4 ▼a Geophysics.
690 ▼a 0373
71020 ▼a University of Michigan. ▼b Atmospheric, Oceanic & Space Science.
7730 ▼t Dissertation Abstracts International ▼g 79-12B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0127
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T15000439 ▼n KERIS ▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다.
980 ▼a 201812 ▼f 2019
990 ▼a ***1012033