Imaging the source regions of the solar wind

Details Imaging the source regions of the solar wind Imaging the source regions of the solar wind

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..385..105r&link_type=abstract

Scientific basis for robotic exploration close to the sun. AIP Conference Proceedings, Volume 385, pp. 105-112 (1997).

Astronomy and Astrophysics

Astronomy

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Astronomical Observations, Remote Observing Techniques

Scientific paper

Remote sensing of the solar corona in the extreme ultraviolet and white light is an indispensable tool for probing the source and acceleration regions of the solar wind which are inaccessible to in situ plasma, particles and fields experiments. Imaging the solar disk and corona 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. The extreme ultraviolet and white light wavelength ranges offer a powerful tool for diagnostic studies of this region.

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