Using the Evolution of Coronal Dimming Regions to Probe the Global Magnetic Field Topology
Open Access
- 27 August 2006
- journal article
- research article
- Published by Springer Science and Business Media LLC in Solar Physics
- Vol. 238 (1), 117-139
- https://doi.org/10.1007/s11207-006-0167-5
Abstract
No abstract availableThis publication has 37 references indexed in Scilit:
- Using Energetic Particles to Probe the Magnetic Topology of EjectaPublished by Wiley ,2013
- Large-Scale Activity in the Bastille Day 2000 Solar EventSolar Physics, 2005
- Transient Coronal Holes as Seen in the Hei1083 nm MLSO ObservationsThe Astrophysical Journal, 2005
- Homologous large‐scale activity in solar eruptive events of 24–26 November 2000Journal of Geophysical Research, 2004
- Large-scale dimmings produced by solar coronal mass ejections according to SOHO/EIT data in four EUV linesAstronomy Reports, 2003
- Weak-Field Magnetogram Calibration using Advanced Stokes Polarimeter Flux Density Maps – II. SOHO/MDI Full-Disk Mode CalibrationSolar Physics, 2003
- Reducing heliospheric magnetic flux from coronal mass ejections without disconnectionJournal of Geophysical Research, 2002
- Plasma and Magnetic Field Inside Magnetic Clouds: a Global StudySolar Physics, 2002
- The structure and origin of magnetic clouds in the solar windAnnales Geophysicae, 1998
- On the Origin of Solar FlaresMonthly Notices of the Royal Astronomical Society, 1960