Bulk properties of the slow and fast solar wind and interplanetary coronal mass ejections measured by Ulysses: Three polar orbits of observations
By R. Ebert, David John McComas, H. Elliott, R. Forsyth, J. Gosling. 2009
137 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/37a8b32ab149097469e960625c6db1b354058135
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In Astronomy and Astrophysics
- S. Cranmer
- C. Chen
- William H. Matthaeus
- Ben Breech
- A. Schekochihin
- Justin C. Kasper
- T. Horbury
- Robert T. Wicks
Citations in the corpus
- EMPIRICAL CONSTRAINTS ON PROTON AND ELECTRON HEATING IN THE FAST SOLAR WIND (2009, background): “This range of values agrees with other exponents reported over these distance that range between about 0.75 and 1 (e.g., Eyni & Steinitz 1981; Lopez & Freeman 1986; Totten et al. 1995; Ebert et al. 2009).”
- Power and spectral index anisotropy of the entire inertial range of turbulence in the fast solar wind (2010, background): “1, the scalings that have been obtained from Ulysses observations (Ebert et al. 2009; Goldstein et al. 1996; Horbury et al. 1996).”