Imperial College London
Alternate

DrRobertForsyth

Faculty of Natural Sciences, Department of Physics

Reader in Space Physics
 
 
 
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Contact

 

+44 (0)20 7594 7761r.forsyth Website

 
 
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Location

 

6M64Huxley BuildingSouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Good:2016:10.1007/s11207-015-0828-3,
author = {Good, SW and Forsyth, RJ},
doi = {10.1007/s11207-015-0828-3},
journal = {Solar Physics},
pages = {239--263},
title = {Interplanetary coronal mass ejections observed by MESSENGER and Venus Express},
url = {http://dx.doi.org/10.1007/s11207-015-0828-3},
volume = {291},
year = {2016}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - Interplanetary coronal mass ejections (ICMEs) observed by the MESSENGER and Venus Express spacecraft have been catalogued and analysed. The ICMEs were identified by a relatively smooth rotation of the magnetic field direction consistent with a flux rope structure, coinciding with a relatively enhanced magnetic field strength. A total of 35 ICMEs were found in the surveyed MESSENGER data (primarily from March 2007 to April 2012), and 84 ICMEs in the surveyed Venus Express data (from May 2006 to December 2013). The ICME flux rope configurations have been determined. Ropes with northward leading edges were about four times more common than ropes with southward leading edges, in agreement with a previously established solar cycle dependence. Ropes with low inclinations to the solar equatorial plane were about four times more common than ropes with high inclinations, possibly an observational effect. Left- and right-handed ropes were observed in almost equal numbers. In addition, data from MESSENGER, Venus Express, STEREO-A, STEREO-B and ACE were examined for multipoint signatures of the catalogued ICMEs. For spacecraft separations below 15° in heliocentric longitude, the second spacecraft observed the ICME flux rope in 82 % of cases; this percentage dropped to 49 % for separations between 15 and 30°, to 18 % for separations between 30 and 45°, and to 12 % for separations between 45 and 60°. As the spacecraft separation increased, it became increasingly likely that only the sheath and not the flux rope of the ICME was observed, in agreement with the notion that ICME flux ropes are smaller in longitudinal extent than the shocks or discontinuities that they often drive. Furthermore, this study has identified 23 ICMEs observed by pairs of spacecraft close to radial alignment. A detailed analysis of these events could lead to a better understanding of how ICMEs evolve during propagation.
AU  - Good,SW
AU  - Forsyth,RJ
DO  - 10.1007/s11207-015-0828-3
EP  - 263
PY  - 2016///
SN  - 1573-093X
SP  - 239
TI  - Interplanetary coronal mass ejections observed by MESSENGER and Venus Express
T2  - Solar Physics
UR  - http://dx.doi.org/10.1007/s11207-015-0828-3
UR  - http://hdl.handle.net/10044/1/28060
VL  - 291
ER  -
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