Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/28987
Title: Assessing the effect of spacecraft motion on single-spacecraft solar wind tracking techniques
Authors: Conlon, Thomas Michael
Milan, Stephen E.
Davies, J. A.
First Published: 1-Oct-2014
Publisher: Springer Netherlands
Citation: Solar Physics, 2014, 289 (10), pp. 3935-3947
Abstract: Recent advances in wide-angle imaging by the Solar Mass Ejection Imager (SMEI) on board the Coriolis spacecraft and more recently by the Heliospheric Imagers (HI) aboard NASA's Solar TErrestrial RElations Observatory (STEREO), have enabled solar wind transients to be imaged and tracked from the Sun to 1 AU and beyond. In this paper we consider two of the techniques that have been used to determine the propagation characteristics of solar wind transients based on single-spacecraft observations, in particular propagation direction and radial speed. These techniques usually assume that the observing spacecraft remains stationary for the duration of observation of the solar wind transient. We determine the inaccuracy introduced by this assumption for the two STEREO spacecraft and find that it can be significant, and it can lead to an overestimation of the transient velocity as seen from STEREO-A and an underestimation as seen by STEREO-B. This has implications for the prediction or solar wind transients at 1 AU and hence is important for the study of space weather.
DOI Link: 10.1007/s11207-014-0549-z
ISSN: 0038-0938
eISSN: 1573-093X
Links: http://link.springer.com/article/10.1007%2Fs11207-014-0549-z
http://hdl.handle.net/2381/28987
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © the authors, 2014. This is an open-access article distributed under the terms of the Creative Commons Attribution License ( http://creativecommons.org/licenses/by/3.0/ ), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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