The plasma Environment of Mars
By A. F. Nagy, D. Winterhalter, Konrad Sauer, T. Cravens, S. Brecht, C. Mazelle, D. Crider, E. Kallio, A. Zakharov, E. Dubinin and 5 more. 2004
314 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/3581799b892b407cb2542a8745db10e41a01dd1f
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
Citations in the corpus
- A review of observed variability in the dayside ionosphere of Mars (2009, background): “…that the intrinsic field, if present at all, is small in comparison to the induced field and that the interaction with the solar wind induces a horizontal magnetic field of about 50 nT throughout the dayside ionosphere (Shinagawa and Cravens, 1992; Nagy et al., 2004 and references therein).”
- Three‐dimensional, multispecies, high spatial resolution MHD studies of the solar wind interaction with Mars (2004, background): “These features are wellknown characteristics of the plasma environment of Mars [cf. Nagy et al., 2004].”
- Influence of the solar EUV flux on the Martian plasma environment (2005, unknown): “The present understanding of this interaction has been recently reviewed by Mazelle et al. (2004) and Nagy et al. (2004).”