The dynamical heliosphere
By Gary Zank, H. Müller. 2001
165 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/8fb1382a0fefb50068957b440034c6686eb38e31
How researchers see this paper
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In Astronomy and Astrophysics
- S. Solanki
- M. Schüssler
- David John McComas
- B. Inhester
- R. Vanderspek
- I. Usoskin
- N. Krivova
- Paul Charbonneau
Citations in the corpus
- INTERSTELLAR GAS FLOW PARAMETERS DERIVED FROM INTERSTELLAR BOUNDARY EXPLORER-Lo OBSERVATIONS IN 2009 AND 2010: ANALYTICAL ANALYSIS (2012, methodology): “For recent overviews of the various modeling methods and their comparison, see, e.g., Fahr et al. (2000), Zank & Müller (2003), Alexashov & Izmodenov (2005), Müller et al. (2008), and Zank et al. (2009).”
- The solar magnetic field (2006, background): “It was shown in model simulations that the front can move within a solar cycle by as much as 10 AU [662, 663].”