Wavelet determination of magnetohydrodynamic-range power spectral exponents in solar wind turbulence seen by Parker Solar Probe
Abstract
Context. The high Reynolds number solar wind flow provides a natural laboratory for the study of turbulence in situ. Parker Solar Probe samples the solar wind between 0.17 AU and 1 AU, providing an opportunity to study how turbulence evolves in the expanding solar wind.
Document Details
- Document Type
- Pub Defense Publication
- Publication Date
- Oct 01, 2023
- Source ID
- 10.1051/0004-6361/202346678
Entities
People
- B. Hnat
- R. O. Dendy
- Sandra Chapman
- X. Wang
Organizations
- Air Force Office of Scientific Research
- Science and Technology Facilities Council