Zobrazeno 1 - 10
of 17
pro vyhledávání: '"L. F. Bargatze"'
Publikováno v:
Annales Geophysicae, Vol 27, Pp 3165-3178 (2009)
We use observations in the solar wind and on the ground to study the interaction of the solar wind and interplanetary magnetic field with Earth's magnetosphere. We find that the type of response depends on the state of the solar wind. Coupling fun
Externí odkaz:
https://doaj.org/article/53706adb8edf40c189d2adf67d79cba0
Autor:
L. F. Bargatze, R. Lee Gordon, Melissa L. Carter, Linda L. Rasmussen, Bruce D. Cornuelle, John A. McGowan, Reinhard E. Flick, Mary Hilbern, James T. Fumo, Bonnie K. Gordon
Publikováno v:
Journal of Geophysical Research: Oceans. 125
Publikováno v:
Earth Science Informatics. 3:127-133
Information is shared within organizations and between organizations at an ever increasing rate. One system design that enables sharing in a distributed environment is a Virtual Observatory. A Virtual Observatory is built with clearly specified and s
Publikováno v:
Annales Geophysicae, Vol 27, Iss 8, Pp 3165-3178 (2009)
Annales Geophysicae, Vol 27, Pp 3165-3178 (2009)
Annales Geophysicae, Vol 27, Pp 3165-3178 (2009)
We use observations in the solar wind and on the ground to study the interaction of the solar wind and interplanetary magnetic field with Earth's magnetosphere. We find that the type of response depends on the state of the solar wind. Coupling functi
Autor:
Patricia H. Reiff, Rumi Nakamura, Oleg Troshichev, L. F. Bargatze, A. A. Petrukovich, T. Nagai, Marc R. Hairston, Toshifumi Mukai, K. B. Baker, M. N. Nozdrachev
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:17299-17310
We study the response of midtail plasma and field parameters to enhanced solar wind electric field input for two substorm intervals on November 22, 1995. The solar wind input signatures were quite different for these two substorms, which had major Pi
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:14583-14599
Variability in the response of the magnetosphere under different interplanetary magnetic field (IMF) conditions is investigated by utilizing a high-resolution, three-dimensional, global magnetohydrodynamic (MHD) model. Changes in the MHD model respon
Autor:
Harlan E. Spence, G Rostoker, Xinlin Li, Daniel N. Baker, L. F. Bargatze, Terrance Onsager, Robert B. Sheldon, Geoffrey D. Reeves, Howard J. Singer, J. B. Blake, R. P. Lepping, Niescja E Turner, R. A. Mewaldt, K. W. Ogilvie, J. H. Allen, Shrikanth Kanekal, Richard D. Belian, Berndt Klecker
Publikováno v:
Journal of Geophysical Research: Space Physics. 102:14141-14148
New, coordinated measurements from the International Solar-Terrestrial Physics (ISTP) constellation of spacecraft are presented to show the causes and effects of recurrent geomagnetic activity during recent solar minimum conditions. It is found using
Publikováno v:
Geophysical Research Letters. 18:151-154
Using three separate but related approaches, the question of whether the dynamic response of the magnetosphere to the solar wind input may be described by a low-order system of equations is examined. First, it is determined that the dimension of the
Publikováno v:
Journal of Geophysical Research. 111
[1] We welcome the comments offered by Haaland et al. [2006] on Bargatze et al. [2005]. Our paper examines a technique developed by Weimer et al. [2003] that can be used to estimate solar wind propagation delay times by applying minimum variance anal
Publikováno v:
Journal of Geophysical Research. 110
[1] We present an evaluation of the Weimer et al. (2003) scheme designed to model interplanetary magnetic field (IMF) phase front propagation in the solar wind. The new method is based on the fact that IMF fluctuations tend to be rotations contained