Zobrazeno 1 - 10
of 1 297
pro vyhledávání: '"SMITH, C W"'
Autor:
Matthaeus, W. H., Adhikari, S., Bandyopadhyay, R., Brown, M. R., Bruno, R., Borovsky, J., Carbone, V., Caprioli, D., Chasapis, A., Chhiber, R., Dasso, S., Dmitruk, P., Del Zanna, L., Dmitruk, P. A., Franci, Luca, Gary, S. P., Goldstein, M. L., Gomez, D., Greco, A., Horbury, T. S., Ji, Hantao, Kasper, J. C., Klein, K. G., Landi, S., Li, Hui, Malara, F., Maruca, B. A., Mininni, P., Oughton, Sean, Papini, E., Parashar, T. N., Pecora, F., Petrosyan, Arakel, Pouquet, Annick, Retino, A., Roberts, Owen, Ruffolo, David, Servidio, Sergio, Spence, Harlan, Smith, C. W., Stawarz, J. E., TenBarge, Jason, Vasquez, B. J., Vaivads, Andris, Valentini, F., Velli, Marco, Verdini, A., Verscharen, Daniel, Whittlesey, Phyllis, Wicks, Robert, Yang, Y., Zimbardo, G.
Space plasmas are three-dimensional dynamic entities. Except under very special circumstances, their structure in space and their behavior in time are not related in any simple way. Therefore, single spacecraft in situ measurements cannot unambiguous
Externí odkaz:
http://arxiv.org/abs/2211.12676
Autor:
Matthaeus, W. H., Bandyopadhyay, R., Brown, M. R., Borovsky, J., Carbone, V., Caprioli, D., Chasapis, A., Chhiber, R., Dasso, S., Dmitruk, P., Del Zanna, L., Dmitruk, P. A., Franci, Luca, Gary, S. P., Goldstein, M. L., Gomez, D., Greco, A., Horbury, T. S., Ji, Hantao, Kasper, J. C., Klein, K. G., Landi, S., Li, Hui, Malara, F., Maruca, B. A., Mininni, P., Oughton, Sean, Papini, E., Parashar, T. N., Petrosyan, Arakel, Pouquet, Annick, Retino, A., Roberts, Owen, Ruffolo, David, Servidio, Sergio, Spence, Harlan, Smith, C. W., Stawarz, J. E., TenBarge, Jason, Vasquez1, B. J., Vaivads, Andris, Valentini, F., Velli, Marco, Verdini, A., Verscharen, Daniel, Whittlesey, Phyllis, Wicks, Robert, Bruno, R., Zimbardo, G.
This paper briefly reviews a number of fundamental measurements that need to be made in order to characterize turbulence in space plasmas such as the solar wind. It has long been known that many of these quantities require simultaneous multipoint mea
Externí odkaz:
http://arxiv.org/abs/1903.06890
Autor:
Desai, M. I., Mason, G. M., Dayeh, M. A., Ebert, R. W., McComas, D. J., Li, G., Cohen, C. M. S., Mewaldt, R. A., Schwadron, N. A., Smith, C. W.
We fit the $\sim$0.1-500 MeV/nucleon H-Fe spectra in 46 large SEP events surveyed by Desai et al. (2016) with the double power-law Band function to obtain a normalization constant, low- and high-energy parameters $\gamma_a$ and $\gamma_b$; and break
Externí odkaz:
http://arxiv.org/abs/1605.03922
Autor:
Bagenal, F., Delamere, P. A., Elliott, H. A., Hill, M. E., Lisse, C. M., McComas, D. J., McNutt, Jr., R. L, Richardson, J. D., Smith, C. W., Strobel, D. F.
The NASA New Horizons spacecraft flies past Pluto on July 14, 2015, carrying two instruments that detect charged particles. Pluto has a tenuous, extended atmosphere that is escaping the weak gravity of the planet. The interaction of the solar wind wi
Externí odkaz:
http://arxiv.org/abs/1509.04660
We report on 49 fast-mode forward shocks propagating inside coronal mass ejections (CMEs) as measured by Wind and ACE at 1 AU from 1997 to 2006. Compared to typical CME-driven shocks, these shocks propagate in different upstream conditions, where the
Externí odkaz:
http://arxiv.org/abs/1503.04141
Publikováno v:
Journal of Geophysical Research, Vol. 115, A02101, 2010
Whether the phenomenology governing MHD turbulence is Kolmogorov or Iroshnikov-Kraichnan (IK) remains an open question, theoretically as well as observationally. The ion heating profile observed in the solar wind provides a quantitative, if indirect,
Externí odkaz:
http://arxiv.org/abs/1106.0530
Publikováno v:
AIP Conf. Proc., 1302, 174-179, 2010
In recent years, a phenomenological solar wind heating model based on a turbulent energy cascade prescribed by the Kolmogorov theory has produced reasonably good agreement with observations on proton temperatures out to distances around 70 AU, provid
Externí odkaz:
http://arxiv.org/abs/1106.0528
Politano and Pouquet's law, a generalization of Kolmogorov's four-fifths law to incompressible MHD, makes it possible to measure the energy cascade rate in incompressible MHD turbulence by means of third-order moments. In hydrodynamics, accurate meas
Externí odkaz:
http://arxiv.org/abs/0901.3499