I
I. Scholl
Researcher at University of Hawaii
Publications - 28
Citations - 486
I. Scholl is an academic researcher from University of Hawaii. The author has contributed to research in topics: Corona & Grid. The author has an hindex of 9, co-authored 26 publications receiving 444 citations. Previous affiliations of I. Scholl include Paris Observatory & Janssen Pharmaceutica.
Papers
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Journal ArticleDOI
Total solar eclipse observations of hot prominence shrouds
S. Rifai Habbal,Miloslav Druckmüller,Huw Morgan,I. Scholl,Vojtech Rušin,Adrian N. Daw,Adrian N. Daw,J. Johnson,Martina B. Arndt +8 more
TL;DR: In this article, the authors show that prominences observed off the solar limb are enshrouded in hot plasmas within twisted magnetic structures, which are referred to as cavities.
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Measuring the solar radius from space during the 2003 and 2006 mercury transits
TL;DR: The Michelson Doppler Imager (MDI) aboard the Solar and Heliospheric Observatory observed the transits of Mercury on 2003 May 7 and 2006 November 8 as discussed by the authors.
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Automatic Detection and Classification of Coronal Holes and Filaments Based on EUV and Magnetogram Observations of the Solar Disk
TL;DR: In this paper, a new method for the automated detection of coronal holes and filaments on the solar disk is presented, where the starting point is coronal images taken by the Extreme Ultraviolet Telescope on the Solar and Heliospheric Observatory (SOHO/EIT) in the Fe ix/x 171 A, Fe xii 195 A, and He ii 304 A extreme ultraviolet (EUV) lines and the corresponding full-disk magnetograms from the Michelson Doppler Imager (SohO/MDI) from different phases of the
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Mapping the Distribution of Electron Temperature and Fe Charge States in the Corona with Total Solar Eclipse Observations
S. Rifai Habbal,Miloslav Druckmüller,Huw Morgan,Adrian N. Daw,Adrian N. Daw,J. Johnson,A. Ding,Martina B. Arndt,Ruth Esser,Vojtech Rušin,I. Scholl +10 more
TL;DR: In this article, the authors show how the 2006 March 29 and 2008 August 1 eclipse observations of a number of Fe emission lines yield an empirical value for a distance, which they call Rt, where the emission changes from being collisionally to radiatively dominated.
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The Precise Solar Shape and Its Variability
TL;DR: Evidence is used from a long-running experiment based in space to show that the Sun’s oblate shape is distinctly constant and almost completely unaffected by the solar-cycle variability seen on its surface.