Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure
By C. Arridge, N. Achilleos, M. Dougherty, K. Khurana, C. Russell. 2006
156 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/885302ad73ff70e1a8755c757cd0f87cdfa8d4d9
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In Astronomy and Astrophysics
- H. Korth
- Sean C. Solomon
- Brian J. Anderson
- R. Winslow
- Catherine L. Johnson
- D. N. Baker
- J. Slavin
- M. Purucker
In Molecular Biology
Citations in the corpus
- Mercury's magnetopause and bow shock from MESSENGER Magnetometer observations (2013, methodology): “, 1997, 2000] as well as the magnetopause of other planets, such as Saturn [Arridge et al., 2006].”
- The Magnetic Field of Mercury (2010, unknown): “Empirical models for the magnetospheric magnetic field analogous to those developed for Earth and other magnetized planets (Khurana 1997; Alexeev and Belenkaya 2005; Arridge et al. 2006; Alexeev et al. 2008) customized for Mercury will therefore remain an important tool.”