Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh21a0393j&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SH21A-0393
Physics
7513 Coronal Mass Ejections, 7594 Instruments And Techniques, 2102 Corotating Streams, 2111 Ejecta, Driver Gases, And Magnetic Clouds, 2164 Solar Wind Plasma
Scientific paper
The Solar Mass Ejection Imager (SMEI) experiment is fixed to the Coriolis spacecraft and views the sky above Earth using sunlight-rejecting baffles and CCD camera technology. SMEI was designed to provide precise photometric white light images over most of the sky on each 102-minute Earth orbit. The brightness sky maps of the inner heliosphere indicate a rich variety of electron density structures that are produced by the material that propagates through it and its interaction with ambient structures. We present some of the preliminary results of the analysis of these photometric SMEI observations derived by 3D reconstructions that allow contaminant signal removal using both interplanetary scintillation (IPS) velocities and SMEI data. We use these analyses to compare preliminary SMEI tomographic white-light results with IPS velocity for the same time intervals.
Buffington Andrew
Hick Pierre P.
Jackson Bernard V.
Kojima Masamichi
Tokumaru Munetoshi
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