Evaluation of the turbulent energy cascade rates from the upper inertial range in the solar wind at 1 AU

By B. Vasquez, Charles W. Smith, Kathleen E. Hamilton, B. T. MacBride, R. Leamon. 2007

142 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/90bc9de2e995e243d88fd0b0160c7c7e0eeba5dd

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. S. Cranmer
2. William H. Matthaeus
3. Ben Breech
4. S. Bale
5. Justin C. Kasper
6. B. T. MacBride
7. Charles W. Smith
8. M. Forman

In Molecular Biology

1. S. Cranmer
2. B. T. MacBride
3. Ben Breech
4. Charles W. Smith
5. William H. Matthaeus
6. Justin C. Kasper
7. R. Howard
8. S. Bale

Citations in the corpus

• The Solar Probe Plus Mission: Humanity’s First Visit to Our Star (2016, background): “This helioradial evolution is evidence for an ongoing non-linear cascade with heating rates estimated to be in the range required to explain the in-situ heating of the solar wind (Vasquez et al. 2007).”
• EMPIRICAL CONSTRAINTS ON PROTON AND ELECTRON HEATING IN THE FAST SOLAR WIND (2009, background): “For electrons,δe is approximately 0.65 at 0.3 AU, it decreases to 0.43 at 1 AU, and to 0.15 at 5 AU.”
• The Turbulent Cascade at 1 AU: Energy Transfer and the Third-Order Scaling for MHD (2007, methodology): “[10] of Vasquez et al. 2007).”