Interplanetary scintillation measurements of the solar wind during Whole Sun Month: Comparisons with coronal and in situ observations
Open Access
- 1 May 1999
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 104 (A5) , 9847-9870
- https://doi.org/10.1029/1998ja900091
Abstract
No abstract availableKeywords
This publication has 38 references indexed in Scilit:
- Magnetohydrodynamic modeling of the solar corona during Whole Sun MonthJournal of Geophysical Research, 1999
- Synoptic Sun during the first Whole Sun Month Campaign: August 10 to September 8, 1996Journal of Geophysical Research, 1999
- Heliospheric tomography using interplanetary scintillation observations: 1. Combined Nagoya and Cambridge dataJournal of Geophysical Research, 1998
- Heliospheric tomography using interplanetary scintillation observations: 3. Correlation between speed and electron density fluctuations in the solar windJournal of Geophysical Research, 1998
- Heliospheric tomography using interplanetary scintillation observations: 2. Latitude and heliocentric distance dependence of solar wind structure at 0.1–1 AUJournal of Geophysical Research, 1998
- Ulysses' return to the slow solar windGeophysical Research Letters, 1998
- SWICS/Ulysses observations: The three‐dimensional structure of the heliosphere in the declining/minimum phase of the solar cycleGeophysical Research Letters, 1997
- Source regions of the slow solar windGeophysical Research Letters, 1997
- Solar wind speed structure in the inner corona at 3–12 RoGeophysical Research Letters, 1995
- Ulysses at 50° south: constant immersion in the high‐speed solar windGeophysical Research Letters, 1994