Solar wind speed structure in the inner corona at 3–12 Ro
- 1 June 1995
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 22 (11) , 1393-1396
- https://doi.org/10.1029/95gl01315
Abstract
No abstract availableThis publication has 26 references indexed in Scilit:
- Density fluctuations in different types of solar wind flow at 1 AU and comparison with results from Doppler scintillation measurements near the SunJournal of Geophysical Research, 1995
- Variation of fractional electron density fluctuations inside 40 Ro observed by Ulysses ranging measurementsGeophysical Research Letters, 1995
- Ulysses at 50° south: constant immersion in the high‐speed solar windGeophysical Research Letters, 1994
- Large-scale solar-wind structure near the Sun detected by Doppler scintillationNature, 1993
- Magnetohydrodynamic simulation of the radial evolution and stream structure of solar-wind turbulencePhysical Review Letters, 1991
- Large-Scale Structure of the Interplanetary MediumPublished by Springer Nature ,1990
- Solar Wind Observations near the SunPublished by Springer Nature ,1986
- Rotational characteristics of the white-light solar corona 1965-1983The Astrophysical Journal, 1984
- Radio wave scattering observations of the solar corona First-order measurements of expansion velocity and turbulence spectrum using Viking and Mariner 10 spacecraftThe Astrophysical Journal, 1981
- Measurements of a solar flare-generated shock wave at 13.1 R0Nature, 1981