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HABBAL, S. MORGAN, H. DRUCKMÜLLER, M. DING, A. COOPER, J. DAW, A. SITTLER, E.
Original Title
Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations
Type
journal article - other
Language
English
Original Abstract
Imaging and spectroscopy of the solar corona, coupled with polarimetry, are the only tools available at present to capture signatures of physical rocesses responsible for coronal heating and solar wind acceleration within the first few solar radii above the solar limb. With the recent advent of mproved detector technology and image processing techniques, broad-band white light and narrow-band multi-wavelength observations of coronal forbidden lines, made during total solar eclipses, have started to yield new views about the thermodynamic and magnetic properties of coronal tructures. This paper outlines these unique capabilities, which until present, have been feasible primarily with observations during natural total solar clipses. This work also draws attention to the exciting possibility of greatly increasing the frequency and duration of solar eclipse observations with Moon orbiting observatories utilizing lunar limb occultation of the solar disk for coronal measurements.
Keywords
Corona , Eclipse, Solar wind
Authors
HABBAL, S.; MORGAN, H.; DRUCKMÜLLER, M.; DING, A.; COOPER, J.; DAW, A.; SITTLER, E.
RIV year
2013
Released
1. 7. 2013
Publisher
Springer
ISBN
0038-0938
Periodical
Solar Physics
Year of study
2013 (285)
Number
1-2
State
Kingdom of the Netherlands
Pages from
9
Pages to
24
Pages count
16
BibTex
@article{BUT94444, author="Shadia Rifai {Habbal} and Huw {Morgan} and Miloslav {Druckmüller} and Adalbert {Ding} and John. F. {Cooper} and Adrian {Daw} and Edward C. {Sittler}", title="Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations", journal="Solar Physics", year="2013", volume="2013 (285)", number="1-2", pages="9--24", issn="0038-0938" }