Zobrazeno 1 - 10
of 193
pro vyhledávání: '"Krupar V"'
Autor:
Dresing, N., Rodríguez-García, L., Jebaraj, I. C., Warmuth, A., Wallace, S., Balmaceda, L., Podladchikova, T., Strauss, R. D., Kouloumvakos, A., Palmroos, C., Krupar, V., Gieseler, J., Xu, Z., Mitchell, J. G., Cohen, C. M. S., de Nolfo, G. A., Palmerio, E., Carcaboso, F., Kilpua, E. K. J., Trotta, D., Auster, U., Asvestari, E., da Silva, D., Dröge, W., Getachew, T., Gómez-Herrero, R., Grande, M., Heyner, D., Holmström, M., Huovelin, J., Kartavykh, Y., Laurenza, M., Lee, C. O., Mason, G., Maksimovic, M., Mieth, J., Murakami, G., Oleynik, P., Pinto, M., Pulupa, M., Richter, I., Rodríguez-Pacheco, J., Sánchez-Cano, B., Schuller, F., Ueno, H., Vainio, R., Vecchio, A., Veronig, A. M., Wijsen, N.
Publikováno v:
A&A 674, A105 (2023)
Context. A solar eruption on 17 April 2021 produced a widespread Solar Energetic Particle (SEP) event that was observed by five longitudinally well-separated observers in the inner heliosphere at heliocentric distances of 0.42 to 1 au: BepiColombo, P
Externí odkaz:
http://arxiv.org/abs/2303.10969
Autor:
Bučík, R., Mason, G. M., Gómez-Herrero, R., Krupar, V., Lario, D., Starkey, M. J., Ho, G. C., Rodríguez-Pacheco, J., Wimmer-Schweingruber, R. F., Lara, F. Espinosa, Tadesse, T., Balmaceda, L., Cohen, C. M. S., Dayeh, M. A., Desai, M. I., Kühl, P., Nitta, N. V., Wiedenbeck, M. E., Xu, Z. G.
Publikováno v:
A&A 669, A13 (2023)
The origin of 3He abundance enhancements in coronal mass ejection (CME)-driven shock gradual solar energetic particle (SEP) events remains largely unexplained. Two mechanisms have been suggested - the re-acceleration of remnant flare material in inte
Externí odkaz:
http://arxiv.org/abs/2210.16403
Autor:
Musset, S., Maksimovic, M., Kontar, E., Krupar, V., Chrysaphi, N., Bonnin, X., Vecchio, A., Cecconi, B., Zaslavsky, A., Issautier, K., Bale, S. D., Pulupa, M.
Publikováno v:
A&A 656, A34 (2021)
We use multi-spacecraft observations of invididual type III radio bursts in order to calculate the directivity of the radio emission, to be compared to the results of ray-tracing simulations of the radio-wave propagation and probe the plasma properti
Externí odkaz:
http://arxiv.org/abs/2109.13713
Autor:
Vecchio, A., Maksimovic, M., Krupar, V., Bonnin, X., Zaslavsky, A., Astier, P. L., Dekkali, M., Cecconi, B., Bale, S. D., Chust, T., Guilhem, E., Khotyaintsev, Yu. V., Krasnoselskikh, V., Kretzschmar, M., Lorfèvre, E., Plettemeier, D., Souček, J., Steller, M., Štverák, Š., Trávníček, P., Vaivads, A.
Publikováno v:
A&A 656, A33 (2021)
In order to allow for a comparison with the measurements from other antenna systems, the voltage power spectral density measured by the Radio and Plasma waves receiver (RPW) on board Solar Orbiter needs to be converted into physical quantities that d
Externí odkaz:
http://arxiv.org/abs/2109.07947
Autor:
Bucik, R., Mason, G. M., Gomez-Herrero, R., Lario, D., Balmaceda, L., Nitta, N. V., Krupar, V., Dresing, N., Ho, G. C., Allen, R. C., Carcaboso, F., Rodriguez-Pacheco, J., Schuller, F., Warmuth, A., Wimmer-Schweingruber, R. F., von Forstner, J. L. Freiherr, Andrews, G. B., Berger, L., Cernuda, I., Lara, F. Espinosa, Lees, W. J., Martin, C., Pacheco, D., Prieto, M., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Tyagi, K., Maksimovic, M., Vecchio, A., Kollhoff, A., Kuhl, P., Xu, Z. G., Eldrum, S.
Publikováno v:
A&A 656, L11 (2021)
We report observations of a relatively long period of 3He-rich solar energetic particles (SEPs) measured by Solar Orbiter. The period consists of several well-resolved ion injections. The high-resolution STEREO-A imaging observations reveal that the
Externí odkaz:
http://arxiv.org/abs/2109.05570
Publikováno v:
Earth Planet. Phys., 4 (2020)
Decametric (DAM) radio emissions are one of the main windows through which one can reveal and understand the Jovian magnetospheric dynamics and its interaction with the moons. DAMs are generated by energetic electrons through cyclotron-maser instabil
Externí odkaz:
http://arxiv.org/abs/2002.01150
Akademický článek
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Autor:
Möstl, C., Isavnin, A., Boakes, P. D., Kilpua, E. K. J., Davies, J. A., Harrison, R. A., Barnes, D., Krupar, V., Eastwood, J. P., Good, S. W., Forsyth, R. J., Bothmer, V., Reiss, M. A., Amerstorfer, T., Winslow, R. M., Anderson, B. J., Philpott, L. C., Rodriguez, L., Rouillard, A. P., Gallagher, P. T., Zhang, T. L.
We present an advance towards accurately predicting the arrivals of coronal mass ejections (CMEs) at the terrestrial planets, including Earth. For the first time, we are able to assess a CME prediction model using data over 2/3 of a solar cycle of ob
Externí odkaz:
http://arxiv.org/abs/1703.00705
We report on our study of radio source regions during the type II radio burst on 2013 May 22 based on direction finding (DF) analysis of the Wind/WAVES and STEREO/WAVES (SWAVES) radio observations at decameter-hectometric (DH) wavelengths. The type I
Externí odkaz:
http://arxiv.org/abs/1606.06989
Akademický článek
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