Zobrazeno 1 - 10
of 458
pro vyhledávání: '"Palmroth M"'
Autor:
Retino, A., Kepko, L., Kucharek, H., Marcucci, M. F., Nakamura, R., Amano, T., Angelopoulos, V., Bale, S. D., Caprioli, D., Cassak, P., Chasapis, A., Chen, L. -J., Dai, L., Dunlop, M. W., Forsyth, C., Fu, H., Galvin, A., Contel, O. Le, Yamauchi, M., Kistler, L., Khotyaintsev, Y., Klein, K., Mann, I. R., Matthaeus, W., Mouikis, K., Nykyri, K., Palmroth, M., Plaschke, F., Saito, Y., Soucek, J., Spence, H., Turner, D. L., Vaivads, A., Valentini, F.
Energetic plasma is everywhere in the Universe. The terrestrial Magnetospheric System is a key case where direct measures of plasma energization and energy transport can be made in situ at high resolution. Despite the large amount of available observ
Externí odkaz:
http://arxiv.org/abs/2311.09920
Autor:
Morosan, D. E., Palmerio, E., Räsänen, J. E., Kilpua, E. K. J., Magdalenić, J., Lynch, B. J., Kumari, A., Pomoell, J., Palmroth, M.
Publikováno v:
A&A 642, A151 (2020)
Context. Coronal mass ejections (CMEs) are large eruptions of magnetised plasma from the Sun that are often accompanied by solar radio bursts produced by accelerated electrons. Aims. A powerful source for accelerating electron beams are CME-driven sh
Externí odkaz:
http://arxiv.org/abs/2008.10245
Publikováno v:
A&A 635, A62 (2020)
Context. Some of the most prominent sources for particle acceleration in our Solar System are large eruptions of magnetised plasma from the Sun called coronal mass ejections (CMEs). These accelerated particles can generate radio emission through vari
Externí odkaz:
http://arxiv.org/abs/2001.08473
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:
FORESAIL collaboration, Palmroth, M., Praks, J., Vainio, R., Janhunen, P., Kilpua, E. K. J., Ganushkina, N. Yu., Afanasiev, A., Ala-Lahti, M., Alho, A., Asikainen, T., Asvestari, E., Battarbee, M., Binios, A., Bosser, A., Brito, T., Envall, J., Ganse, U., George, H., Gieseler, J., Good, S., Grandin, M., Haslam, S., Hedman, H. -P., Hietala, H., Jovanovic, N., Kakakhel, S., Kalliokoski, M., Kettunen, V. V., Koskela, T., Lumme, E., Meskanen, M., Morosan, D., Mughal, M. Rizwan, Niemelä, P., Nyman, S., Oleynik, P., Osmane, A., Palmerio, E., Pfau-Kempf, Y., Peltonen, J., Plosila, J., Polkko, J., Poluianov, S., Pomoell, J., Price, D., Punkkinen, A., Punkkinen, R., Riwanto, B., Salomaa, L., Slavinskis, A., Säntti, T., Tammi, J., Tenhunen, H., Toivanen, P., Tuominen, J., Turc, L., Valtonen, E., Virtanen, P., Westerlund, T.
Today, the near-Earth space is facing a paradigm change as the number of new spacecraft is literally sky-rocketing. Increasing numbers of small satellites threaten the sustainable use of space, as without removal, space debris will eventually make ce
Externí odkaz:
http://arxiv.org/abs/1905.09600
Autor:
Palmroth, M., Tapio, J., Soucek, A., Perrels, A., Jah, M., Lönnqvist, M., Nikulainen, M., Piaulokaite, V., Seppälä, T., Virtanen, J.
Publikováno v:
In Space Policy August 2021 57
Akademický článek
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Publikováno v:
Journal of Geophysical Research: Space Physics, 119, 6273, 2014
Magnetic reconnection (MR) is a key physical concept explaining the addition of magnetic flux to the magnetotail and closed flux lines back-motion to the dayside magnetosphere. This scenario elaborated by \citet{dung63}, can explain many aspects of s
Externí odkaz:
http://arxiv.org/abs/1411.7927
Akademický článek
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Publikováno v:
Computer Physics Communications, Volume 184, Issue 4, April 2013, Pages 1297-1309
We present an easy to use and flexible grid library for developing highly scalable parallel simulations. The distributed cartesian cell-refinable grid (dccrg) supports adaptive mesh refinement and allows an arbitrary C++ class to be used as cell data
Externí odkaz:
http://arxiv.org/abs/1212.3496