Zobrazeno 1 - 10
of 235
pro vyhledávání: '"Kronberg, E. A."'
Prediction and understanding of soft proton contamination in XMM-Newton: a machine learning approach
Autor:
Kronberg, E. A., Gastaldello, F., Haaland, S., Smirnov, A., Berrendorf, M., Ghizzardi, S., Kuntz, K. D., Sivadas, N., Allen, R. C., Tiengo, A., Ilie, R., Huang, Y., Kistler, L.
One of the major and unfortunately unforeseen sources of background for the current generation of X-ray telescopes are few tens to hundreds of keV (soft) protons concentrated by the mirrors. One such telescope is the European Space Agency's (ESA) X-r
Externí odkaz:
http://arxiv.org/abs/2009.13156
Autor:
Branduardi-Raymont, G., Berthomier, M., Bogdanova, Y., Carter, J. C., Collier, M., Dimmock, A., Dunlop, M., Fear, R., Forsyth, C., Hubert, B., Kronberg, E., Laundal, K. M., Lester, M., Milan, S., Oksavik, K., Østgaard, N., Palmroth, M., Plaschke, F., Porter, F. S., Rae, I. J., Read, A., Samsonov, A., Sembay, S., Shprits, Y., Sibeck, D. G., Walsh, B., Yamauchi, M.
This paper addresses the fundamental science question: "How does solar wind energy flow through the Earth's magnetosphere, how is it converted and distributed?". We need to understand how the Sun creates the heliosphere, and how the planets interact
Externí odkaz:
http://arxiv.org/abs/1908.04730
Autor:
Kronberg, E. A., Grigorenko, E. E., Haaland, S. E., Daly, P. W., Delcourt, D. C., Luo, H., Kistler, L. M., Dandouras, I.
The spatial distributions of different ion species are useful indicators for plasma sheet dynamics. In this statistical study based on 7 years of Cluster observations, we establish the spatial distributions of oxygen ions and protons at energies from
Externí odkaz:
http://arxiv.org/abs/1606.01652
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Autor:
Blöcker, A., Kronberg, E. A., Grigorenko, E. E., Roussos, E., Clark, G., 1 Department of Earth and Environmental Sciences Ludwig Maximilian University of Munich Munich Germany, 2 Space Research Institute Russian Academy of Sciences Moscow Russia, 3 Max Planck Institute for Solar System Research Göttingen Germany, 4 Johns Hopkins University Applied Physics Laboratory Laurel MD USA
Energetic particle acceleration and energization in planetary magnetotails are often associated with dipolarization fronts characterized by a rapid increase of the meridional component of the magnetic field. Despite many studies of dipolarization eve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::304a68674bc7dc3b8909f4eb1a08718c
http://resolver.sub.uni-goettingen.de/purl?gldocs-11858/10733
http://resolver.sub.uni-goettingen.de/purl?gldocs-11858/10733
Publikováno v:
Space Weather: The International Journal of Research & Applications; Sep2023, Vol. 21 Issue 9, p1-20, 20p
Publikováno v:
Kinematics and Physics of Celestial Bodies
Autor:
Blöcker, A., Kronberg, E. A., Grigorenko, E. E., Clark, G., Kozak, L., Vogt, M. F., Roussos, E., 1 Department of Earth and Environmental Sciences Ludwig‐Maximilians‐University Munich Germany, 2 Space Research Institute Russian Academy of Sciences Moscow Russia, 3 Johns Hopkins University Applied Physics Laboratory Laurel MD USA, 4 Astronomy and Space Physics Department Kyev Taras Shevchenko University Kyev Ukraine, 5 Center for Space Physics Boston University Boston MA USA, 6 Max Planck Institute for Solar System Research Göttingen Germany
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Transient magnetic reconnection plays an important role in energetic particle acceleration in planetary magnetospheres. Jupiter's magnetosphere provides a unique natural laboratory to study processes of energy transport and transformation. Strong ele
Akademický článek
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