Zobrazeno 1 - 10
of 1 487
pro vyhledávání: '"Forsyth, R. J."'
Autor:
Kilpua, E. K. J., Good, S. W., Dresing, N., Vainio, R., Davies, E. E., Forsyth, R. J., Gieseler, J., Lavraud, B., Asvestari, E., Morosan, D. E., Pomoell, J., Price, D. J., Heyner, D., Horbury, T. S., Angelini, V., O'Brien, H., Evans, V., Rodriguez-Pacheco, J., Herrero, R. Gómez, Ho, G. C., Wimmer-Schweingruber, R.
Sheaths ahead of coronal mass ejections (CMEs) are large heliospheric structures that form with CME expansion and propagation. Turbulent and compressed sheaths contribute to the acceleration of particles in the corona and in interplanetary space, but
Externí odkaz:
http://arxiv.org/abs/2112.09472
Autor:
Davies, E. E., Möstl, C., Owens, M. J., Weiss, A. J., Amerstorfer, T., Hinterreiter, J., Bauer, M., Bailey, R. L., Reiss, M. A., Forsyth, R. J., Horbury, T. S., O'Brien, H., Evans, V., Angelini, V., Heyner, D., Richter, I., Auster, H-U., Magnes, W., Baumjohann, W., Fischer, D., Barnes, D., Davies, J. A., Harrison, R. A.
Publikováno v:
A&A 656, A2 (2021)
On 2020 April 19 a coronal mass ejection (CME) was detected in situ by Solar Orbiter at a heliocentric distance of about 0.8 AU. The CME was later observed in situ on April 20th by the Wind and BepiColombo spacecraft whilst BepiColombo was located ve
Externí odkaz:
http://arxiv.org/abs/2012.07456
We present observations of the same magnetic cloud made near Earth by the Advance Composition Explorer (ACE), Wind, and the Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon's Interaction with the Sun (ARTEMIS) mission comprising
Externí odkaz:
http://arxiv.org/abs/2009.09896
Interplanetary coronal mass ejections (ICMEs) are a significant feature of the heliospheric environment and the primary cause of adverse space weather at the Earth. ICME propagation, and the evolution of ICME magnetic field structure during propagati
Externí odkaz:
http://arxiv.org/abs/1905.07227
The B-field structures of two ICMEs each observed by a pair of spacecraft close to radial alignment have been analysed. The ICMEs were observed in situ by MESSENGER and STEREO-B in Nov. 2010 and Nov. 2011, while the spacecraft were separated by more
Externí odkaz:
http://arxiv.org/abs/1802.04004
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
Autor:
Good, S. W., Forsyth, R. J.
Interplanetary coronal mass ejections (ICMEs) observed by the MESSENGER (MES) and Venus Express (VEX) spacecraft have been catalogued and analysed. The ICMEs were identified by a relatively smooth rotation of the magnetic field direction consistent w
Externí odkaz:
http://arxiv.org/abs/1511.07749
Publikováno v:
Journal of the Royal Statistical Society. Series C (Applied Statistics), 1999 Jan 01. 48(4), 427-439.
Externí odkaz:
https://www.jstor.org/stable/2680754
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