D
D. M. Rust
Researcher at American Science and Engineering, Inc.
Publications - 22
Citations - 1898
D. M. Rust is an academic researcher from American Science and Engineering, Inc.. The author has contributed to research in topics: Solar flare & Corona. The author has an hindex of 17, co-authored 22 publications receiving 1857 citations.
Papers
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Journal ArticleDOI
An emerging flux model for the solar flare phenomenon
TL;DR: In this paper, an outline of the physical processes involved in the emerging flux model, which appears to explain naturally many solar flare observations, is presented, and it is suggested that a (small) simple loop flare occurs if the new flux appears in a region where no great amount of magnetic energy in excess of potential is stored.
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The origin and development of the May 1997 magnetic cloud
David F. Webb,R. P. Lepping,L. F. Burlaga,Craig DeForest,Davin Larson,Sara F. Martin,Simon Plunkett,D. M. Rust +7 more
TL;DR: In this article, a complete halo coronal mass ejection (CME) was observed by the SOHO Large Angle and Spectrometric Coronagraph (LASCO) coronagraphs on May 12, 1997.
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Origin and location of the hard X-ray emission in a two-ribbon flare
P. Hoyng,André Duijveman,Marcos E. Machado,D. M. Rust,Z. Svestka,A. Boelee,C. de Jager,K. T. Frost,H. Lafleur,G. M. Simnett,H. F. van Beek,Bruce E. Woodgate +11 more
TL;DR: In this paper, the authors report observations on the two-ribbon flare of 1980 May 21 by the Hard X-Ray Imaging Spectrometer, the H..cap alpha.. and magnetic field data.
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Expansion of an X-ray coronal arch into the outer corona
D. M. Rust,E. Hildner +1 more
TL;DR: An asymmetric, expanding arch, photographed in the inner corona with an X-ray telescope on 13 August, 1973, is identified as the source of the mass ejected in a white light transient in the outer corona as discussed by the authors.
Journal ArticleDOI
Coronal X-ray enhancements associated with H-alpha filament disappearances
TL;DR: The Skylab/ATM experiment as mentioned in this paper provided high-resolution soft X-ray images of the lower corona away from active regions, revealing frequent large-scale transient Xray enhancements which could often be associated with the disappearance of H-alpha filaments.