Zobrazeno 1 - 10
of 148
pro vyhledávání: '"W J, Hughes"'
Publikováno v:
Journal of Geophysical Research: Space Physics. 120:8723-8737
Using a global multifluid MHD model, we demonstrate the effects of magnetospheric O+ on bursty magnetotail flows. We carry out two simulations without ionospheric outflow to use as baseline, one driven by real solar wind data and one driven by ideali
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 83:32-38
We present results from a new magnetohydrodynamic (MHD) model of the inner heliosphere. The model is adapted from the well-established Lyon–Fedder–Mobarry (LFM) MHD simulation code, which until recently mostly applied to studies of the terrestria
Autor:
W. J. Hughes, D.L. Murr
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 69:223-233
This study seeks to establish a new system characteristic describing dayside convective flows in the coupled magnetosphere–ionosphere: the low-pass filter function through which interplanetary magnetic field (IMF) fluctuations are processed as they
Autor:
Stanley W. H. Cowley, Christopher J. Owen, W. J. Hughes, L. Newitt, Mitchell J. Brittnacher, J. F. Watermann, T. J. Hughes, William S. Kurth, David J. McComas, H. Khan, Geoffrey D. Reeves, E. Kolesnikova, M. Lester, Charles W. Smith, David J. Southwood, Howard J. Singer
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:30141-30175
During the Earth swing-by of the Cassini spacecraft, a worldwide program of data-gathering was undertaken to define the prevailing interplanetary and geophysical conditions. This included observations of the interplanetary medium, outer magnetosphere
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 63:1609-1621
Results of the study of two substorms from Interball auroral UV measurements and two-dimensional patterns of equivalent ionospheric currents derived from the MACCS/CANOPUS and Greenland magnetometer arrays are presented. Substorm development in 2-D e
Autor:
D. L. Murr, W. J. Hughes
Publikováno v:
Geophysical Research Letters. 28:2145-2148
Changes in ionospheric flow patterns provide direct observations of how the magnetosphere-ionosphere system is coupled to the IMF. The nature and location of reconnection on the magnetopause is communicated to the ionosphere, which responds by reconf
Electrodynamics of the poleward auroral border observed by Polar during a substorm on April 22, 1998
Autor:
Daniel M. Ober, Christopher T. Russell, N. C. Maynard, William J. Burke, W. J. Hughes, John B. Sigwarth, W. K. Peterson, L. A. Frank, J. D. Scudder
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:5927-5943
Observations from Polar during a substorm on April 22, 1998, are used to specify electrodynamic characteristics of the high-latitude auroral boundary on the nightside. Polar was moving equatorward near invariant latitude 72°, 2305 magnetic local tim
Autor:
Chao-Song Huang, George J. Sofko, J. W. MacDougall, V. O. Papitashvili, D. André, W. J. Hughes, A. V. Kustov
Publikováno v:
Geophysical Research Letters. 27:1795-1798
It has been observed that quasi-periodic oscillations in the solar wind and interplanetary magnetic field (IMF) can result in the generation of auroral electrojet bursts and gravity waves with a similar period. In this paper, we present radar and mag
Autor:
T. J. Hughes, K. I. Paularena, Eftyhia Zesta, A. J. Lazarus, Mark J. Engebretson, W. J. Hughes
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:28041-28058
On November 9, 1993, at around 1715 UT, a strong and well-structured traveling convection vortex (TCV) event occurred and was observed by the Magnetometer Array for Cusp and Cleft Studies (MACCS) and the Canadian Auroral Network for the OPEN Program
Autor:
V. Pilipenko, Dmitry Baishev, E. S. Barkova, J. L. Posch, S. I. Solovyev, Mark J. Engebretson, W. J. Hughes, Kiyohumi Yumoto
Publikováno v:
Scopus-Elsevier
By comparing data from a globally distributed set of high-latitude magnetic observatories with optical data in the nightside auroral ionosphere, we studied the features of short-term activations (≤10–15 min) during periods of steady magnetospheri