Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Kuehl, Patrick"'
Autor:
Jebaraj, Immanuel C., Dresing, Nina, Krasnoselskikh, Vladimir, Agapitov, Oleksiy V., Gieseler, Jan, Trotta, Domenico, Wijsen, Nicolas, Larosa, Andrea, Kouloumvakos, Athanasios, Palmroos, Christian, Dimmock, Andrew, Kolhoff, Alexander, Kuehl, Patrick, Fleth, Sebastian, Fedeli, Annamaria, Valkila, Saku, Lario, David, Khotyaintsev, Yuri V., Vainio, Rami
Collisionless shock waves have long been considered amongst the most prolific particle accelerators in the universe. Shocks alter the plasma they propagate through and often exhibit complex evolution across multiple scales. Interplanetary (IP) travel
Externí odkaz:
http://arxiv.org/abs/2311.05765
Autor:
Gastaldello, Fabio, Marelli, Martino, Molendi, Silvano, Bartalucci, Iacopo, Kühl, Patrick, Grant, Catherine E., Ghizzardi, Simona, Rossetti, Mariachiara, De Luca, Andrea, Tiengo, Andrea
We analyzed the unexposed to the sky outFOV region of the MOS2 detector on board XMM-Newton covering 15 years of data amounting to 255 Ms. We show convincing evidence that the origin of the unfocused background in XMM-Newton is due to energetic proto
Externí odkaz:
http://arxiv.org/abs/2202.05286
Autor:
Marelli, Martino, Molendi, Silvano, Rossetti, Mariachiara, Gastaldello, Fabio, Salvetti, David, De Luca, Andrea, Bartalucci, Iacopo, Kühl, Patrick, Esposito, Paolo, Ghizzardi, Simona, Tiengo, Andrea
Our understanding of the background of the EPIC/pn camera onboard XMM-Newton is incomplete. This affects the study of extended sources and can influence the predictions of the background of future X-ray missions. We provide new results based on the a
Externí odkaz:
http://arxiv.org/abs/2012.02071
Autor:
Whitman, Kathryn, Egeland, Ricky, Richardson, Ian G., Allison, Clayton, Quinn, Philip, Barzilla, Janet, Kitiashvili, Irina, Sadykov, Viacheslav, Bain, Hazel M., Dierckxsens, Mark, Mays, M. Leila, Tadesse, Tilaye, Lee, Kerry T., Semones, Edward, Luhmann, Janet G., Núñez, Marlon, White, Stephen M., Kahler, Stephen W., Ling, Alan G., Smart, Don F., Shea, Margaret A., Tenishev, Valeriy, Boubrahimi, Soukaina F., Aydin, Berkay, Martens, Petrus, Angryk, Rafal, Marsh, Michael S., Dalla, Silvia, Crosby, Norma, Schwadron, Nathan A., Kozarev, Kamen, Gorby, Matthew, Young, Matthew A., Laurenza, Monica, Cliver, Edward W., Alberti, Tommaso, Stumpo, Mirko, Benella, Simone, Papaioannou, Athanasios, Anastasiadis, Anastasios, Sandberg, Ingmar, Georgoulis, Manolis K., Ji, Anli, Kempton, Dustin, Pandey, Chetraj, Li, Gang, Hu, Junxiang, Zank, Gary P., Lavasa, Eleni, Giannopoulos, Giorgos, Falconer, David, Kadadi, Yash, Fernandes, Ian, Dayeh, Maher A., Muñoz-Jaramillo, Andrés, Chatterjee, Subhamoy, Moreland, Kimberly D., Sokolov, Igor V., Roussev, Ilia I., Taktakishvili, Aleksandre, Effenberger, Frederic, Gombosi, Tamas, Huang, Zhenguang, Zhao, Lulu, Wijsen, Nicolas, Aran, Angels, Poedts, Stefaan, Kouloumvakos, Athanasios, Paassilta, Miikka, Vainio, Rami, Belov, Anatoly, Eroshenko, Eugenia A., Abunina, Maria A., Abunin, Artem A., Balch, Christopher C., Malandraki, Olga, Karavolos, Michalis, Heber, Bernd, Labrenz, Johannes, Kühl, Patrick, Kosovichev, Alexander G., Oria, Vincent, Nita, Gelu M., Illarionov, Egor, O’Keefe, Patrick M., Jiang, Yucheng, Fereira, Sheldon H., Ali, Aatiya, Paouris, Evangelos, Aminalragia-Giamini, Sigiava, Jiggens, Piers, Jin, Meng, Lee, Christina O., Palmerio, Erika, Bruno, Alessandro, Kasapis, Spiridon, Wang, Xiantong, Chen, Yang, Sanahuja, Blai, Lario, David, Jacobs, Carla, Strauss, Du Toit, Steyn, Ruhann, van den Berg, Jabus, Swalwell, Bill, Waterfall, Charlotte, Nedal, Mohamed, Miteva, Rositsa, Dechev, Momchil, Zucca, Pietro, Engell, Alec, Maze, Brianna, Farmer, Harold, Kerber, Thuha, Barnett, Ben, Loomis, Jeremy, Grey, Nathan, Thompson, Barbara J., Linker, Jon A., Caplan, Ronald M., Downs, Cooper, Török, Tibor, Lionello, Roberto, Titov, Viacheslav, Zhang, Ming, Hosseinzadeh, Pouya
Publikováno v:
In Advances in Space Research 15 December 2023 72(12):5161-5242
Autor:
Kühl, Patrick, Heber, Bernd, Gómez-Herrero, Raúl, Malandraki, Olga, Posner, Arik, Sierks, Holger
The near-Earth energetic particle environment has been monitored since the 1970's. With the increasing importance of quantifying the radiation risk for, e.g. for the human exploration of the Moon and Mars, it is essential to continue and further impr
Externí odkaz:
http://arxiv.org/abs/2010.00864
Autor:
Guo, Jingnan, Zeitlin, Cary, Wimmer-Schweingruber, Robert F., McDole, Thoren, Kuehl, Patrick, Appel, Jan C., Matthiae, Daniel, Krauss, Johannes, Koehler, Jan
For future human missions to Mars, it is important to study the surface radiation environment during extreme and elevated conditions. In the long term, it is mainly Galactic Cosmic Rays (GCRs) modulated by solar activity that contributes to the radia
Externí odkaz:
http://arxiv.org/abs/1705.06763
The Sun is an effective particle accelerator producing solar energetic particle (SEP) events during which particles up to several GeVs can be observed. Those events observed at Earth with the neutron monitor network are called ground level enhancemen
Externí odkaz:
http://arxiv.org/abs/1611.03289
Autor:
Wiengarten, Tobias, Kleimann, Jens, Fichtner, Horst, Kühl, Patrick, Kopp, Andreas, Heber, Bernd, Kissmann, Ralf
Publikováno v:
The Astrophysical Journal, Volume 788, Issue 1, article id. 80, 16 pp. (2014)
The transport of energetic particles such as Cosmic Rays is governed by the properties of the plasma being traversed. While these properties are rather poorly known for galactic and interstellar plasmas due to the lack of in situ measurements, the he
Externí odkaz:
http://arxiv.org/abs/1406.0293
Akademický článek
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Autor:
Jung, Alexander1 (AUTHOR) Alexander.Jung@ecb.europa.eu, Kuehl, Patrick2 (AUTHOR)
Publikováno v:
Scottish Journal of Political Economy. Jul2021, Vol. 68 Issue 3, p298-321. 24p. 8 Charts, 5 Graphs.