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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Journal ArticleDOI
Penetrating particle ANalyzer (PAN)
Xin Wu,G. Ambrosi,P. Azzarello,Benedikt Bergmann,B. Bertucci,B. Bertucci,Franck Cadoux,M. Campbell,M. Duranti,Maria Ionica,Merlin Kole,Säm Krucker,Säm Krucker,Gunnar Maehlum,Dirk Meier,M. Paniccia,L. S. Pinsky,C. Plainaki,Stanislav Pospisil,Timo A. Stein,Pierre Alexandre Thonet,Nicola Tomassetti,Nicola Tomassetti,Andrii Tykhonov +23 more
TL;DR: PAN as mentioned in this paper is a scientific instrument suitable for deep space and interplanetary missions, which can precisely measure and monitor the flux, composition, and direction of highly penetrating particles in deep space, over at least one full solar cycle (11 years).
Journal ArticleDOI
Multiwavelength Stereoscopic Observation of the 2013 May 1 Solar Flare and CME
Erica Lastufka,Säm Krucker,Ivan Zimovets,B. A. Nizamov,Stephen M. White,Satoshi Masuda,D. Golovin,Maxim Litvak,I. G. Mitrofanov,A. B. Sanin +9 more
TL;DR: In this article, the authors investigated the RHESSI-observed occulted hard X-ray emissions that originated at least 0.1 RS above the flare site and revealed a hot, extended (11 MK, > 60 arcsec) thermal source from the escaping CME core, with densities around 10 cm−3.
Journal ArticleDOI
Solar Energetic Electron Events Associated with Hard X-Ray Flares
Penetrating Particle Analyzer (pan)
Xin Wu,B. Bertucci,Lawrence Pinsky,Giovanni Ambrosi,Dirk Meier,Gunnar Maehlum,Philip Azzarello,Benedikt Bergmann,Michael Campbell,Merlin Kole,Säm Krucker,M. Paniccia,Stanislav Pospisil,Pierre Alexandre Thonet,Andrii Tykhonov,Timo A. Stein +15 more
Journal ArticleDOI
Physics of ion acceleration in the solar flare on 2005 September 7 determines γ-ray and neutron production
Kyoko Watanabe,Robert P. Lin,Säm Krucker,Ronald J. Murphy,Gerald H. Share,M. J. Harris,M. Gros,Yasushi Muraki,Takashi Sako,Yutaka Matsubara,T. Sakai,Shoichi Shibata,J. F. Valdés-Galicia,Luis Xavier Gonzalez,A. Hurtado,O. Musalem,P. Miranda,N. Martinic,R. Ticona,A. Velarde,Fumio Kakimoto,Yoshiki Tsunesada,H. Tokuno,Shoichi Ogio +23 more
TL;DR: Hua et al. as mentioned in this paper analyzed the data using the solar-flare magnetic-loop transport and interaction model and found that the model could successfully fit the data with intermediate values of loop magnetic convergence and pitch-angle scattering parameters.