Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Frederic Effenberger"'
Publikováno v:
Earth and Space Science, Vol 6, Iss 10, Pp 2000-2015 (2019)
Solar wind observations show that geomagnetic storms are mainly driven by interplanetary coronal mass ejections (ICMEs) and corotating or stream interaction regions (C/SIRs). We present a binary classifier that assigns one of these drivers to 7,546 s
Externí odkaz:
https://doaj.org/article/3fde4b2ce4d443aabed14a325479b524
The transport of cosmic rays in turbulent magnetic fields is commonly investigated by solving the Newton-Lorentz equation of test particles in synthetic turbulence fields. These fields are typically generated from superpositions of Fourier modes with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::18aab76129c2e1aae31b7e8cd6d9b3cd
https://doi.org/10.5194/egusphere-egu23-14458
https://doi.org/10.5194/egusphere-egu23-14458
Publikováno v:
Journal of Geophysical Research: Space Physics. 128
Autor:
Kathryn Whitman, Ricky Egeland, Ian G. Richardson, Clayton Allison, Philip Quinn, Janet Barzilla, Irina Kitiashvili, Viacheslav Sadykov, Hazel M. Bain, Mark Dierckxsens, M. Leila Mays, Tilaye Tadesse, Kerry T. Lee, Edward Semones, Janet G. Luhmann, Marlon Núñez, Stephen M. White, Stephen W. Kahler, Alan G. Ling, Don F. Smart, Margaret A. Shea, Valeriy Tenishev, Soukaina F. Boubrahimi, Berkay Aydin, Petrus Martens, Rafal Angryk, Michael S. Marsh, Silvia Dalla, Norma Crosby, Nathan A. Schwadron, Kamen Kozarev, Matthew Gorby, Matthew A. Young, Monica Laurenza, Edward W. Cliver, Tommaso Alberti, Mirko Stumpo, Simone Benella, Athanasios Papaioannou, Anastasios Anastasiadis, Ingmar Sandberg, Manolis K. Georgoulis, Anli Ji, Dustin Kempton, Chetraj Pandey, Gang Li, Junxiang Hu, Gary P. Zank, Eleni Lavasa, Giorgos Giannopoulos, David Falconer, Yash Kadadi, Ian Fernandes, Maher A. Dayeh, Andrés Muñoz-Jaramillo, Subhamoy Chatterjee, Kimberly D. Moreland, Igor V. Sokolov, Ilia I. Roussev, Aleksandre Taktakishvili, Frederic Effenberger, Tamas Gombosi, Zhenguang Huang, Lulu Zhao, Nicolas Wijsen, Angels Aran, Stefaan Poedts, Athanasios Kouloumvakos, Miikka Paassilta, Rami Vainio, Anatoly Belov, Eugenia A. Eroshenko, Maria A. Abunina, Artem A. Abunin, Christopher C. Balch, Olga Malandraki, Michalis Karavolos, Bernd Heber, Johannes Labrenz, Patrick Kühl, Alexander G. Kosovichev, Vincent Oria, Gelu M. Nita, Egor Illarionov, Patrick M. O’Keefe, Yucheng Jiang, Sheldon H. Fereira, Aatiya Ali, Evangelos Paouris, Sigiava Aminalragia-Giamini, Piers Jiggens, Meng Jin, Christina O. Lee, Erika Palmerio, Alessandro Bruno, Spiridon Kasapis, Xiantong Wang, Yang Chen, Blai Sanahuja, David Lario, Carla Jacobs, Du Toit Strauss, Ruhann Steyn, Jabus van den Berg, Bill Swalwell, Charlotte Waterfall, Mohamed Nedal, Rositsa Miteva, Momchil Dechev, Pietro Zucca, Alec Engell, Brianna Maze, Harold Farmer, Thuha Kerber, Ben Barnett, Jeremy Loomis, Nathan Grey, Barbara J. Thompson, Jon A. Linker, Ronald M. Caplan, Cooper Downs, Tibor Török, Roberto Lionello, Viacheslav Titov, Ming Zhang, Pouya Hosseinzadeh
Publikováno v:
Advances in Space Research.
Solar Energetic Particles (SEP) events are interesting from a scientific perspective as they are the product of a broad set of physical processes from the corona out through the extent of the heliosphere, and provide insight into processes of particl
Autor:
Shaela I. Jones, D. Folta, O. C. StCyr, Frederic Effenberger, Sami K. Solanki, V. J. Sterken, Bernd Heber, Jan Staub, R. D. Strauss, Olga E. Malandraki, Achim Gandorfer, Patrick Kühl, Carl J. Henney, Arik Posner, Johann Hirzberger, C. N. Arge
Publikováno v:
Space Weather, 19 (9)
The Earth-Sun Lagrangian point 4 is a meta-stable location at 1 AU from the Sun, 60° ahead of Earth's orbit. It has an uninterrupted view of the solar photosphere centered on W60, the Earth's nominal magnetic field connection to the Sun. Such a miss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6213397b07c19c3b3c791541240f936
https://hdl.handle.net/20.500.11850/505514
https://hdl.handle.net/20.500.11850/505514
Publikováno v:
Physics of Plasmas. 29:072302
We study the process of nonlinear shock acceleration based on a nonlinear diffusion–advection equation. The nonlinearity is introduced via a dependence of the spatial diffusion coefficient on the distribution function of accelerating particles. Thi
Autor:
Arik Posner, Charles Nickolos Arge, Jan Staub, Orville C StCyr, David C Folta, Sami K. Solanki, Roelf Du Toit Strauss, Frederic Effenberger, Achim Gandorfer, Bernd Heber, Carl John Henney, Johann Hirzberger, Shaela Jones, Patrick Kuehl, Olga Malandraki, Veerle J Sterken
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::45f321757cec97915f7253ecb6436c90
https://doi.org/10.1002/essoar.10506845.1
https://doi.org/10.1002/essoar.10506845.1
Autor:
Alexander Warmuth, Nina Dresing, Maximilian Bruedern, Ludwig Klein, Frederic Effenberger, Sophie Musset, Lindsay Glesener
In-situ observations of solar energetic particle events are determined by a combination of acceleration, injection, and transport processes which are often hard to disentangle. However, the energy spectrum of impulsive electron events is believed to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1033706950699343fe1c2e4271dcdeac
https://doi.org/10.5194/egusphere-egu21-9543
https://doi.org/10.5194/egusphere-egu21-9543
Autor:
Irina Zhelavskaya, Frederic Effenberger, Dedong Wang, Hayley Allison, Sebastian Cervantes, Yuri Shprits, Alexander Drozdov, Angelica Castillo, Nikita Aseev
Using the three-dimensional Versatile Electron Radiation Belt (VERB-3D) code, we perform simulations to investigate the dynamic evolution of relativistic electrons in the Earth’s outer radiation belt. In our simulations, we use data from the Geosta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::27ff3669f9f16dce6212b4bce11fd02e
https://doi.org/10.5194/egusphere-egu21-3802
https://doi.org/10.5194/egusphere-egu21-3802
The basics of focused transport as applied to solar energetic particles are reviewed, paying special attention to areas of common misconception. The micro-physics of charged particles interacting with slab turbulence are investigated to illustrate th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdfb35512e6cdeb5be85a93819f3a07c
http://arxiv.org/abs/2012.07570
http://arxiv.org/abs/2012.07570