Sector boundary transformation by an open magnetic cloud
Open Access
- 1 November 1998
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (A11) , 26859-26868
- https://doi.org/10.1029/98ja02391
Abstract
No abstract availableKeywords
This publication has 35 references indexed in Scilit:
- Solar cycle evolution of the structure of magnetic clouds in the inner heliosphereGeophysical Research Letters, 1998
- Central axial field direction in magnetic clouds and its relation to southward interplanetary magnetic field events and dependence on disappearing solar filamentsJournal of Geophysical Research, 1998
- Tracing the topology of the October 18–20, 1995, magnetic cloud with ∼0.1–10² keV electronsGeophysical Research Letters, 1997
- Solar wind streamer belt structureJournal of Geophysical Research, 1996
- Magnetic cloud‐bow shock interaction: WIND and IMP‐8 observationsGeophysical Research Letters, 1996
- Large‐scale properties and solar connection of the heliospheric current and plasma sheets: WIND observationsGeophysical Research Letters, 1996
- Effect of coronal mass ejections on the structure of the heliospheric current sheetJournal of Geophysical Research, 1996
- The determination of interplanetary magnetic field polarities around sector boundaries using E > 2 keV electronsGeophysical Research Letters, 1994
- A test of source‐surface model predictions of heliospheric current sheet inclinationJournal of Geophysical Research, 1994
- Field line draping about fast coronal mass ejecta: A source of strong out‐of‐the‐ecliptic interplanetary magnetic fieldsGeophysical Research Letters, 1987