The spatial structure of the oncoming solar wind at Earth and the shortcomings of a solar-wind monitor at L1-Reference-Cited by-同舟云学术

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The spatial structure of the oncoming solar wind at Earth and the shortcomings of a solar-wind monitor at L1

Published:2018-10 Issue: Volume:177 Page:2-11
ISSN:1364-6826
Container-title:Journal of Atmospheric and Solar-Terrestrial Physics
language:en
Short-container-title:Journal of Atmospheric and Solar-Terrestrial Physics

Author:

Borovsky Joseph E.

Funder

Space Science Institute

NASA Heliophysics LWS TRT program

NASA Heliophysics Guest Investigator Program

NSF GEM Program

Publisher

Elsevier BV

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference104 articles.

1. Channeled propagation of solar particles;Anderson;Inter. Cosm. Ray Conf.,1985

2. Observation of flux-tube crossings in the solar wind;Arnold;Astrophys. J.,2013

3. Anisotropic cosmic radiation fluxes of solar origin;Bartley;J. Geophys. Res.,1966

4. Comparisons between two wavelet functions in extracting coherent structures from solar wind time series;Bolzan;Braz. J. Phys.,2009

5. The flux-tube texture of the solar wind: strands of the magnetic carpet at 1 AU?;Borovsky;J. Geophys. Res.,2008

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2. PRIME: a probabilistic neural network approach to solar wind propagation from L1;Frontiers in Astronomy and Space Sciences;2023-09-19

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