Zobrazeno 1 - 10
of 2 247
pro vyhledávání: '"Dougherty M"'
Autor:
Masters, A., Sulaiman, A. H., Stawarz, Ł., Reville, B., Sergis, N., Fujimoto, M., Burgess, D., Coates, A. J., Dougherty, M. K.
A leading explanation for the origin of Galactic cosmic rays is acceleration at high-Mach number shock waves in the collisionless plasma surrounding young supernova remnants. Evidence for this is provided by multi-wavelength non-thermal emission thou
Externí odkaz:
http://arxiv.org/abs/1705.11096
Autor:
Yao, Zhonghua, Coates, A. J., Ray, L. C., Rae, I. J., Grodent, D., Jones, G. H., Dougherty, M. K., Owen, C. J., Guo, R. L., Dunn, W., Radioti, A., Pu, Z. Y., Lewis, G. R., Waite, J. H., Gerard, J. -C.
Publikováno v:
The Astrophysical Journal Letters, 846(2):L25
Using measurements from the Cassini spacecraft in Saturn's magnetosphere, we propose a 3D physical picture of a corotating reconnection site, which can only be driven by an internally generated source. Our results demonstrate that the corotating magn
Externí odkaz:
http://arxiv.org/abs/1701.04559
Autor:
Hadid, L. Z., Sahraoui, F., Kiyani, K. H., Retinò, A., Modolo, R., Canu, P., Masters, A., Dougherty, M. K.
Low frequency turbulence in Saturn's magnetosheath is investigated using in-situ measurements of the Cassini spacecraft. Focus is put on the magnetic energy spectra computed in the frequency range $\sim[10^{-4}, 1]$Hz. A set of 42 time intervals in t
Externí odkaz:
http://arxiv.org/abs/1611.08245
Autor:
Stephan, K., Roatsch, T., Tosi, F., Matz, K.-D., Kersten, E., Wagner, R., Molyneux, P., Palumbo, P., Poulet, F., Hussmann, H., Barabash, S., Bruzzone, L., Dougherty, M., Gladstone, R., Gurvits, L.I., Hartogh, P., Iess, L., Wahlund, J.-E., Wurz, P., Witasse, O., Grasset, O., Altobelli, N., Carter, J., Cavalié, T., d'Aversa, E., Della Corte, V., Filacchione, G., Galli, A., Galluzzi, V., Gwinner, K., Hauber, E., Jaumann, R., Krohn, K., Langevin, Y., Lucchetti, A., Migliorini, A., Piccioni, G., Solomonidou, A., Stark, A., Tobie, G., Tubiana, C., Vallat, C., Van Hoolst, T.
Publikováno v:
In Planetary and Space Science 15 November 2021 208