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 Article
Heating events in the quiet solar corona : multiwavelength correlations
Arnold O. Benz,Säm Krucker +1 more
TL;DR: In this article, the Fourier transform in time is found to have steeper spectra in the corona and upper chromosphere than in the transition region, and the temporal sequence of brightenings has been determined by cross-correlations of identical picture elements in different emissions.
Journal ArticleDOI
The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action
I. Zouganelis,A. De Groof,Andrew Walsh,David R. Williams,Daniel Mueller,O. C. St. Cyr,F. Auchere,David Berghmans,Andrzej Fludra,Timothy S. Horbury,R. A. Howard,Säm Krucker,Milan Maksimovic,Christopher J. Owen,J. Rodriiguez-Pacheco,Marco Romoli,Sami K. Solanki,C. Watson,L. Sanchez,J. Lefort,Pedro Osuna,Holly Gilbert,Teresa Nieves-Chinchilla,Lucia Abbo,Olga Alexandrova,Anastasios Anastasiadis,V. Andretta,Ester Antonucci,T. Appourchaux,Angels Aran,C. N. Arge,Guillaume Aulanier,D. N. Baker,Stuart D. Bale,Marina Battaglia,L. R. Bellot Rubio,Alessandro Bemporad,M. Berthomier,Karine Bocchialini,Xavier Bonnin,A. S. Brun,Roberto Bruno,Eric Buchlin,J. Buechner,Radoslav Bučík,Fernando Carcaboso,R. Carr,I. Carrasco-Blazquez,Baptiste Cecconi,I. Cernuda Cangas,Christopher H. K. Chen,Lakshmi Pradeep Chitta,Thomas Chust,Kévin Dalmasse,Raffaella D'Amicis,V. Da Deppo,R. De Marco,S. Dolei,L. Dolla,T. Dudok de Wit,L. van Driel-Gesztelyi,Jonathan Eastwood,F. Espinosa Lara,Laszlo Istvan Etesi,Andrei Fedorov,F. Felix-Redondo,Silvano Fineschi,B. Fleck,Dominique Fontaine,N. J. Fox,Achim Gandorfer,Vincent Génot,Manolis K. Georgoulis,S. Gissot,A. Giunta,Laurent Gizon,Raul Gomez-Herrero,C. Gontikakis,Gary Graham,Lucie M. Green,T. Grundy,M. Haberreiter,L. K. Harra,Donald M. Hassler,Johann Hirzberger,George C. Ho,G. J. Hurford,Davina Innes,K. Issautier,Alexander W. James,Nils Janitzek,Miho Janvier,Natasha L. S. Jeffrey,Jack Jenkins,Y. V. Khotyaintsev,Karl-Ludwig Klein,Eduard P. Kontar,Ioannis Kontogiannis,C. Krafft,V. Krasnoselskikh,Matthieu Kretzschmar,Nicolas Labrosse,Andreas Lagg,Federico Landini,Benoit Lavraud,I. Leon,Susan T. Lepri,Gethyn R. Lewis,P. C. Liewer,Jon A. Linker,Stefano Livi,David Long,P. Louarn,Olga Malandraki,Shane A. Maloney,V. Martinez-Pillet,Mihailo M. Martinović,Arnaud Masson,Sarah A. Matthews,Lorenzo Matteini,Nicole Meyer-Vernet,Kostas Moraitis,Richard Morton,Sophie Musset,Georgios Nicolaou,Alexander Nindos,Helen O'Brien,D. Orozco Suárez,Mathew J. Owens,Maurizio Pancrazzi,Athanasios Papaioannou,S. Parenti,Etienne Pariat,S. Patsourakos,Denise Perrone,Hardi Peter,Rui Pinto,Christina Plainaki,Dirk Plettemeier,Simon Plunkett,Jim M. Raines,N. E. Raouafi,Hamish A. S. Reid,Alessandro Retinò,Laurence Rezeau,P. Rochus,L. Rodriguez,L. Rodriguez-Garcia,Markus Roth,A. P. Rouillard,F. Sahraoui,Clementina Sasso,Jesper Schou,Udo H. Schuehle,Luca Sorriso-Valvo,Jan Soucek,Daniele Spadaro,Marco Stangalini,David Stansby,M. Steller,Antoine Strugarek,Štěpán Štverák,Roberto Susino,Daniele Telloni,C. Terasa,Luca Teriaca,Sergio Toledo-Redondo,J. C. del Toro Iniesta,Georgia Tsiropoula,A. Tsounis,Kostas Tziotziou,Francesco Valentini,Andris Vaivads,Alberto Vecchio,Marco Velli,Cis Verbeeck,Andrea Verdini,Daniel Verscharen,N. Vilmer,Angelos Vourlidas,Robert T. Wicks,Robert F. Wimmer-Schweingruber,Thomas Wiegelmann,Peter R. Young,Andrei Zhukov +184 more
TL;DR: In this paper, a Science Activity Plan (SAP) is developed to address the top-level science questions such as: (1) What drives the solar wind and where does the coronal magnetic field originate? (2) How do solar transients drive heliospheric variability? (3)How do solar eruptions produce energetic particle radiation that fills the heliosphere? (4) How does the solar dynamo work and drive connections between the Sun and the helIosphere?
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Hard x-rays associated with type iii radio bursts
TL;DR: In this article, the WAVES instrument on WIND observed six interplanetary type III radio bursts, one approximately every 2 minutes, and each was accompanied by a weak hard X-ray (HXR) burst (12-15 keV) observed by RHESSI.
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Studies of Microflares in RHESSI Hard X-Ray, Big Bear Solar Observatory Hα, and Michelson Doppler Imager Magnetograms
TL;DR: In this paper, the morphology of 12 microflares jointly observed by RHESSI in the energy range from 3 to 15 keV and by Big Bear Solar Observatory (BBSO) at the Hα line was studied.
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PITCH-ANGLE DISTRIBUTIONS AND TEMPORAL VARIATIONS OF 0.3-300 keV SOLAR IMPULSIVE ELECTRON EVENTS
TL;DR: In this article, the authors investigate the propagation of ~0.3-300 keV electrons in five solar impulsive electron events, observed by the WIND three-dimensional Plasma and Energetic Particle instrument, that have rapid-rise and rapid-decay temporal profiles.