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HABBAL, S. MORGAN, H. DRUCKMÜLLER, M. DING, A. COOPER, J. DAW, A. SITTLER, E.
Originální název
Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations
Typ
článek v časopise - ostatní, Jost
Jazyk
angličtina
Originální abstrakt
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.
Klíčová slova
Corona , Eclipse, Solar wind
Autoři
HABBAL, S.; MORGAN, H.; DRUCKMÜLLER, M.; DING, A.; COOPER, J.; DAW, A.; SITTLER, E.
Rok RIV
2013
Vydáno
1. 7. 2013
Nakladatel
Springer
ISSN
0038-0938
Periodikum
Solar Physics
Ročník
2013 (285)
Číslo
1-2
Stát
Nizozemsko
Strany od
9
Strany do
24
Strany počet
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" }