MHD-scale anisotropy in solar wind turbulence near the Sun using Parker solar probe data
Author:
Affiliation:
1. Department of Physics, Indian Institute of Technology, Kanpur , 208016, India
2. Department of Astrophysical Sciences, Princeton University , Princeton, NJ 08544, USA
Abstract
Funder
NASA
DST
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stac1449/43892940/stac1449.pdf
Reference77 articles.
1. Highly structured slow solar wind emerging from an equatorial coronal hole
2. The FIELDS Instrument Suite for Solar Probe Plus
3. Geometry of Magnetic Fluctuations near the Sun from the Parker Solar Probe
4. Solar Wind Turbulence Studies Using MMS Fast Plasma Investigation Data
5. Enhanced Energy Transfer Rate in Solar Wind Turbulence Observed near the Sun from Parker Solar Probe
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