Lancaster EPrints

A statistical comparison of solar wind propagation delays derived from multi-spacecraft techniques

Case, Nathan and Wild, James (2012) A statistical comparison of solar wind propagation delays derived from multi-spacecraft techniques. Journal of Geophysical Research, 117 (A2). ISSN 0148-0227

PDF - Published Version
Download (1763Kb) | Preview


    We present a large-scale statistical study of the solar wind prop- agnation delay between NASA’s Advanced Composition Explorer spacecraft and ESA’s Cluster 1 spacecraft. This study focuses on those periods when Cluster was within the unimpeded solar wind, upstream of the bow shock nose, between 2001 and 2010. Using a cross-correlation method to compare the ACE and Cluster data, nearly 5000 propagation delays have been calculated and compared to both corresponding propagation delays in the OMNIweb dataset and to those computed by a simple “flat” (i.e. distance/speed) propagation model. The results show that statistically there is little difference between the OMNI and flat propagation delay times and that the cross-correlation method agrees well with both, but there are times when the various methods give significantly different propagation estimates. There is found to be no influence on the relationship between the estimated and observed solar wind propagation delays from the solar wind speed or IMF orientation.

    Item Type: Journal Article
    Journal or Publication Title: Journal of Geophysical Research
    Additional Information: ©2012. American Geophysical Union. All Rights Reserved.
    Departments: Faculty of Science and Technology > Physics
    ID Code: 52252
    Deposited By: ep_importer_pure
    Deposited On: 09 Jan 2012 11:53
    Refereed?: Yes
    Published?: Published
    Last Modified: 20 Jun 2018 00:18
    Identification Number:

    Actions (login required)

    View Item