INTERSTELLAR GAS FLOW PARAMETERS DERIVED FROM INTERSTELLAR BOUNDARY EXPLORER-Lo OBSERVATIONS IN 2009 AND 2010: ANALYTICAL ANALYSIS

By E. Möbius, P. Bochsler, M. Bzowski, D. Heirtzler, M. Kubiak, H. Kucharek, M. Lee, T. Leonard, N. Schwadron, X. Wu and 8 more. 2012

166 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/32f3e3bbf03b52356490b7856a022aea3ef59ac2

How researchers see this paper

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In Astronomy and Astrophysics

1. William H. Matthaeus
2. Gary Zank
3. P. Isenberg
4. N. Lugaz
5. H. Spence
6. D. N. Baker
7. L. Kistler
8. M. Horányi

In Atmospheric Science

1. William H. Matthaeus

Citations in the corpus

• NEUTRAL INTERSTELLAR HELIUM PARAMETERS BASED ON IBEX-Lo OBSERVATIONS AND TEST PARTICLE CALCULATIONS (2012, methodology): “Therefore, drawing meaningful conclusions about this interstellar species is possible only after critical evaluation of the flow of NISHe gas, which is a topic of this paper as well as some other papers in this special issue (Möbius et al. 2012; Lee et al. 2012).”
• Interstellar Mapping and Acceleration Probe (IMAP): A New NASA Mission (2018, methodology): “Improvements in these observations are essential because, prior to IMAP, direct measurement of ISN atoms by IBEX (McComas et al. 2012; Möbius et al. 2009, 2012; Bzowski et al. 2012) and from Ulysses (Witte 2004) along with direction determinations by PUIs (Drews et al. 2012) presented flow speed…”