202 citations · 496 across the 11 of their papers we have counts for
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Evaluation of CME Arrival Prediction Using Ensemble Modeling Based on Heliospheric Imaging Observations
Tanja Amerstorfer, Jürgen Hinterreiter, Martin A. Reiss +8
In this study, we evaluate a coronal mass ejection (CME) arrival prediction tool that utilizes the wide-angle observations made by STEREO's heliospheric imagers (HI). The unsurpass…
Forecasting the Ambient Solar Wind with Numerical Models: I. On the Implementation of an Operational Framework
Martin A. Reiss, Peter J. MacNeice, Leila M. Mays +4
The ambient solar wind conditions in interplanetary space and in the near-Earth environment are determined by activity on the Sun. Steady solar wind streams modulate the propagatio…
Tracking and Validating ICMEs Propagating Toward Mars Using STEREO Heliospheric Imagers Combined With Forbush Decreases Detected by MSL/RAD
Johan L. Freiherr von Forstner, Jingnan Guo, Robert F. Wimmer-Schweingruber +7
The Radiation Assessment Detector (RAD) instrument onboard the Mars Science Laboratory (MSL) mission's Curiosity rover has been measuring galactic cosmic rays (GCR) as well as sola…
Generic magnetic field intensity profiles of interplanetary coronal mass ejections at Mercury, Venus and Earth from superposed epoch analyses
Miho Janvier, Reka Winslow, Simon Good +8
We study interplanetary coronal mass ejections (ICMEs) measured by probes at different heliocentric distances (0.3-1AU) to investigate the propagation of ICMEs in the inner heliosp…
The Magnetic Field Geometry of Small Solar Wind Flux Ropes Inferred from their Twist Distribution
W. Yu, C. J. Farrugia, N. Lugaz +4
This work extends recent efforts on the force-free modeling of large flux rope-type structures (magnetic clouds, MCs) to much smaller spatial scales. We first select small flux rop…
Correlation of ICME Magnetic Fields at Radially Aligned Spacecraft
S. W. Good, R. J. Forsyth, J. P. Eastwood +1
The B-field structures of two ICMEs each observed by a pair of spacecraft close to radial alignment have been analysed. The ICMEs were observed in situ by MESSENGER and STEREO-B in…