The WHI Corona from Differential Emission Measure Tomography
- 10 February 2011
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 274 (1-2) , 259-284
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This publication has 41 references indexed in Scilit:
- THE SOLAR MINIMUM CORONA FROM DIFFERENTIAL EMISSION MEASURE TOMOGRAPHYThe Astrophysical Journal, 2010
- STEREOSCOPIC POLAR PLUME RECONSTRUCTIONS FROMSTEREO/SECCHI IMAGESThe Astrophysical Journal, 2009
- The Physical Properties of Coronal Streamers. II.The Astrophysical Journal, 2007
- Ion Temperatures in the Quiet Solar CoronaThe Astrophysical Journal, 2007
- Stagnation Flow in Thin Streamer BoundariesThe Astrophysical Journal, 2005
- Oxygen Abundance in Coronal StreamersThe Astrophysical Journal, 2005
- The Effect of Proton Temperature Anisotropy on the Solar Minimum Corona and WindThe Astrophysical Journal, 2003
- The inner solar corona seen by SUMER, LASCO/C1, and EIT: Electron densities and temperatures during the rise of the new solar cycleAstronomy & Astrophysics, 2002
- Properties of Quiet-Sun Coronal Plasmas at Distances of 1.03 ⩽ R☉ ⩽ 1.50 along the Solar Equatorial PlaneThe Astrophysical Journal, 1999
- Solar minimum streamer densities and temperatures using Whole Sun Month coordinated data setsJournal of Geophysical Research, 1999