Role of solar wind turbulence in the coupling of the solar wind to the Earth's magnetosphere

By J. Borovsky, H. Funsten. 2003

156 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/a73726552988f826ca821a27f060b97f9a90311a

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

1. B. Lavraud
2. E. Kilpua
3. R. Steiger
4. A. Balogh
5. Ying Liu
6. J. Borovsky

In Molecular Biology

1. B. Lavraud
2. E. Kilpua
3. A. Balogh
4. R. Steiger
5. Ying Liu
6. J. Borovsky

Citations in the corpus

• Altered solar wind-magnetosphere interaction at low Mach numbers: Coronal mass ejections (2008, background): “This property is also likely to change the interaction of low Mach number CMEs with the magnetosphere [e.g., Borovsky and Funsten, 2003].”
• Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, background): “Rapid IMF fluctuations in sheaths, CIRS and HSSs can also enhance viscous interactions at the magnetopause as demonstrated e.g., by Borovsky and Funsten (2003) and Osmane et al. (2015) and lead to larger geoeffectivity.”