Coronal structure inferred from remote sensing observations

Details Coronal structure inferred from remote sensing observations Coronal structure inferred from remote sensing observations

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..385....9f&link_type=abstract

Scientific basis for robotic exploration close to the sun. AIP Conference Proceedings, Volume 385, pp. 9-16 (1997).

Astronomy and Astrophysics

Astronomy

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

Scientific paper

Remote-sensing observations of the Sun and inner heliosphere are reviewed to appraise our understanding of the mix of mechanisms that heat the corona and accelerate the solar wind. An assessment of experimental uncertainties and the basic assumptions needed to translate measurables into physical models, reveals very large fundamental uncertainties in our knowledge of coronal structure near the Sun. We develop a time-dependent, filamentary model of the extended corona that is consistent with a large number of remote sensing observations of the solar atmosphere and the solar wind.

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