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Arrival Time Calculation for Interplanetary Coronal Mass Ejections with Circular Fronts and Application to STEREO Observations of the 2009 February 13 Eruption
DOI: 10.1088/0004-637X/741/1/34 Bibcode: 2011ApJ...741...34M

Luhmann, J. G.; Zhang, T. L.; Möstl, C. +11 more

One of the goals of the NASA Solar TErestrial RElations Observatory (STEREO) mission is to study the feasibility of forecasting the direction, arrival time, and internal structure of solar coronal mass ejections (CMEs) from a vantage point outside the Sun-Earth line. Through a case study, we discuss the arrival time calculation of interplanetary C…

2011 The Astrophysical Journal
VenusExpress 58
Deriving the Physical Parameters of a Solar Ejection with an Isotropic Magnetohydrodynamic Evolutionary Model
DOI: 10.1088/0004-637X/741/1/47 Bibcode: 2011ApJ...741...47B

Vourlidas, Angelos; Stenborg, Guillermo; Berdichevsky, Daniel B.

The time-space evolution of a ~50° wide coronal mass ejection (CME) on 2007 May 21 is followed remotely with the Solar Terrestrial Relations Observatory heliospheric imager HI-1, and measured in situ near Venus by the MESSENGER and Venus-Express spacecraft. The paper compares the observations of the CME structure with a simple, analytical magnetoh…

2011 The Astrophysical Journal
VenusExpress 6