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Remote Sensing Measurements of the Corona with the Solar Probe

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dc.contributor.author Habbal, Shadia Rifai en_US
dc.contributor.author Woo, Richard en_US
dc.date.accessioned 2004-10-01T06:02:48Z
dc.date.available 2004-10-01T06:02:48Z
dc.date.issued 1996 en_US
dc.identifier.clearanceno 96-1612 en_US
dc.identifier.uri http://hdl.handle.net/2014/27570
dc.description.abstract Remote sensing measurements of the solar corona are indespensible for the exploration of the source and acceleration regions of the solar wind which are inaccessible to in situ plasma, paritcles and field experiments.Furthermore, imaging the solar disk and coronal from the unique vantage point of the trajectory and the proximity of the Solar Probe spacecraft, will provide the first ever opportunity to explore the small scale structures within coronal holes and streamers from viewing angles and with spatial resolutions never attained before. en_US
dc.format.extent 425331 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other remote sensing solar wind solar corona situ plasma Solar Probe coronal holes coronal streamerssoalr imagers en_US
dc.title Remote Sensing Measurements of the Corona with the Solar Probe en_US


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