S
Säm Krucker
Researcher at University of California, Berkeley
Publications - 394
Citations - 20683
Säm Krucker is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Solar flare & Flare. The author has an hindex of 65, co-authored 372 publications receiving 18539 citations. Previous affiliations of Säm Krucker include Kyung Hee University & ETH Zurich.
Papers
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Hard X-ray and metric/decimetric spatially resolved observations of the 10 April 2002 solar flare
TL;DR: In this paper, the authors discuss the temporal evolution of X-ray sources together with the evolution of the radio emission sites observed at different coronal heights by the Nancay Radioheliograph (NRH).
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Hard X-Ray Constraints on Small-Scale Coronal Heating Events
Andrew J. Marsh,David M. Smith,Lindsay Glesener,James A. Klimchuk,Stephen J. Bradshaw,Juliana Vievering,Iain G. Hannah,Steven Christe,Shin-nosuke Ishikawa,Säm Krucker,Säm Krucker +10 more
TL;DR: In this paper, the authors analyzed data from the Focusing Optics X-ray Solar Imager (FOXSI) and the Nuclear Spectroscopic Telescope Array (NuSTAR) spacecraft to constrain properties of AR nanoflares simulated by the EBTEL field-line-averaged hydrodynamics code.
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RHESSI IMAGING SURVEY OF γ-RAY BREMSSTRAHLUNG EMISSION IN SOLAR FLARES
Shin-Ichi Ishikawa,Shin-Ichi Ishikawa,Säm Krucker,Tadayuki Takahashi,Tadayuki Takahashi,Robert P. Lin,Robert P. Lin +6 more
TL;DR: In this article, the authors presented a high-energy (>150 keV) imaging survey of all solar γ-ray flares observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) to study bremsstrahlung emission from relativistic electrons.
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Joint hard X-ray observations with ASO-S/HXI and SO/STIX
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Energy Deposition and Hard X-Ray Source Motions in the 2002 July 23 γ-Ray Flare
TL;DR: In this article, the authors derived and investigated for the first time the correlation between cumulative deposited energy at the footpoints and their separation and showed an excellent correlation for most of the time intervals, however, despite the good correlation, the derived amount of released magnetic energy is far too small to account for the energy in HXR-producing electrons.