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dc.contributor.author Bisi, M. M.
dc.contributor.author Jackson, B. V.
dc.contributor.author Hick, P. P.
dc.contributor.author Buffington, A.
dc.contributor.author Clover, J. M.
dc.contributor.author Tokumaru, M.
dc.contributor.author Fujiki, K.
dc.date.accessioned 2013-07-13T03:52:48Z
dc.date.available 2013-07-13T03:52:48Z
dc.date.issued 2010-06-01
dc.identifier.citation Bisi , M M , Jackson , B V , Hick , P P , Buffington , A , Clover , J M , Tokumaru , M & Fujiki , K 2010 , ' Three-Dimensional Reconstructions and Mass Determination of the 2008 June 2 LASCO Coronal Mass Ejection using STELab Interplanetary Scintillation Observations ' Astrophysical Journal Letters , vol 715 , no. 2 , pp. L104-L108 . DOI: 10.1088/2041-8205/715/2/L104 en
dc.identifier.issn 2041-8213
dc.identifier.other PURE: 259464
dc.identifier.other PURE UUID: 9b1a278f-9b13-40dd-ae50-0d41ac32a78f
dc.identifier.other RAD: 5835
dc.identifier.other RAD_Outputs_All_ID_Import_20121105.csv: row: 2491
dc.identifier.other Bibtex: urn:fff96963e71860d4f05902dd40a7d758
dc.identifier.other Scopus: 77952825734
dc.identifier.other handle.net: 2160/8529
dc.identifier.uri http://hdl.handle.net/2160/8529
dc.identifier.uri http://iopscience.iop.org/2041-8205/715/2/L104 en
dc.description.abstract We examine and reconstruct the interplanetary coronal mass ejection (ICME) first seen in space-based coronagraph white-light difference images on 2008 June 1 and 2. We use observations of interplanetary scintillation (IPS) taken with the Solar-Terrestrial Environment Laboratory (STELab), Japan, in our three-dimensional (3D) tomographic reconstruction of density and velocity. The coronal mass ejection (CME) was first observed by the LASCO C3 instrument at around 04:17 UT on 2008 June 2. Its motion subsequently moved across the C3 field of view with a plane-of-the-sky velocity of 192 km s–1. The 3D reconstructed ICME is consistent with the trajectory and extent of the CME measurements taken from the CDAW CME catalog. However, excess mass estimates vary by an order of magnitude from Solar and Heliospheric Observatory and Solar Terrestrial Relations Observatory coronagraphs to our 3D IPS reconstructions of the inner heliosphere. We discuss the discrepancies and give possible explanations for these differences as well as give an outline for future studies. en
dc.language.iso eng
dc.relation.ispartof Astrophysical Journal Letters en
dc.rights en
dc.subject solar wind en
dc.subject Sun: coronal mass ejections (CMEs) en
dc.title Three-Dimensional Reconstructions and Mass Determination of the 2008 June 2 LASCO Coronal Mass Ejection using STELab Interplanetary Scintillation Observations en
dc.type /dk/atira/pure/researchoutput/researchoutputtypes/contributiontojournal/article en
dc.identifier.doi https://doi.org/10.1088/2041-8205/715/2/L104
dc.contributor.institution Department of Physics en
dc.description.status Peer reviewed en


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