Zobrazeno 1 - 10
of 70
pro vyhledávání: '"Terry G. Forbes"'
Autor:
Yuhao Chen, Jing Ye, Zhixing Mei, Chengcai Shen, Ilia I. Roussev, Terry G. Forbes, Jun Lin, Udo Ziegler
Publikováno v:
The Astrophysical Journal. 933:148
We performed 2D magnetohydrodynamical numerical experiments to study the response of the coronal magnetic configuration to the newly emerging magnetic flux. The configuration includes an electric-current-carrying flux rope modeling the prominence flo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::839c1b29fedd262d5d0ab9e7fc4dbe44
https://doi.org/10.3847/1538-4357/ac73ef
https://doi.org/10.3847/1538-4357/ac73ef
Autor:
Rumi Nakamura, Robert E. Ergun, C. J. Pollock, Christopher T. Russell, Charlie J. Farrugia, Per-Arne Lindqvist, Noé Lugaz, Kristoff Paulson, Barry Mauk, Roy B. Torbert, S. A. Fuselier, D. J. Gershman, J. R. Shuster, Robert J. Strangeway, B. Lavraud, Ian J. Cohen, L. Alm, A. J. Rogers, Bernard J. Vasquez, Yuri V. Khotyaintsev, Göran Marklund, D. Payne, Barbara L. Giles, Matthew R. Argall, Hiroshi Matsui, James L. Burch, Fausto T. Gratton, S. M. Petrinec, Terry G. Forbes
Publikováno v:
Journal of Geophysical Research: Space Physics. 123:8983-9004
In this paper we report on a sequence of large-amplitude Alfvenic fluctuations terminating in a field and flow discontinuity and their effects on electromagnetic fields and plasmas in the near-magn ...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::febaa31a271b8d7a22a3abaeac116565
https://doi.org/10.1029/2018ja025724
https://doi.org/10.1029/2018ja025724
Autor:
James L. Burch, Roy B. Torbert, I. Dors, Kevin Genestreti, Terry G. Forbes, Charlie J. Farrugia, Matthew R. Argall, Robert J. Strangeway, Barbara L. Giles
A method is described to model the magnetic field in the vicinity of constellations of multiple satellites using field and plasma current measurements. This quadratic model has the properties that the divergence is zero everywhere and matches the mea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0eb97af64efd0b4828455557d99ffcf5
http://arxiv.org/abs/1909.11255
http://arxiv.org/abs/1909.11255
Autor:
Per-Arne Lindqvist, A. C. Rager, James L. Burch, Barbara L. Giles, John C. Dorelli, Frederick Wilder, Terry G. Forbes, Yu. V. Khotyaintsev, Roy B. Torbert, Robert E. Ergun, L. Alm, Robert J. Strangeway, Matthew R. Argall, Charlie J. Farrugia, Narges Ahmadi
Publikováno v:
Journal of Geophysical Research: Space Physics. 122
On 22 October 2016, the Magnetospheric Multiscale (MMS) spacecraft encountered the electron diffusion region (EDR) when the magnetosheath field was southward, and there were signatures of fast reco ...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::237919123a35067c7f3ce41790a88c60
https://doi.org/10.1002/2017ja024579
https://doi.org/10.1002/2017ja024579
Autor:
Terry G. Forbes, Dana Longcope
Publikováno v:
Solar Physics. 289:2091-2122
We present a simplified analytic model of a quadrupolar magnetic field and flux rope to model coronal mass ejections. The model magnetic field is two-dimensional, force-free and has current only on the axis of the flux rope and within two currents sh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da55ce7e6d37ae6b7f1e72645336b6b7
https://doi.org/10.1007/s11207-013-0464-8
https://doi.org/10.1007/s11207-013-0464-8
Publikováno v:
The Astrophysical Journal. 722:329-342
Supra-arcade downflows (SADs) have been observed with Yohkoh/SXT (soft X-rays (SXR)), TRACE (extreme ultra-violet (EUV)), SoHO/LASCO (white light), SoHO/SUMER (EUV spectra), and Hinode/XRT (SXR). Characteristics such as low emissivity and trajectorie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1ca107f750b0e7a8c9de27de1955859
https://doi.org/10.1088/0004-637x/722/1/329
https://doi.org/10.1088/0004-637x/722/1/329
Publikováno v:
The Astrophysical Journal. 721:1547-1558
We investigate coronal energy flow during a simulated coronal mass ejection (CME). We model the CME in the context of the global corona using a 2.5D numerical MHD code in spherical coordinates that includes coronal heating, thermal conduction, and ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0c0537633a77627c5b265e2105eb12e0
https://doi.org/10.1088/0004-637x/721/2/1547
https://doi.org/10.1088/0004-637x/721/2/1547
Publikováno v:
The Astrophysical Journal. 858:70
Using a recently developed analytical procedure, we determine the rate of magnetic reconnection in the "standard" model of eruptive solar flares. During the late phase, the neutral line is located near the lower tip of the reconnection current sheet,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fef7ff71b3b7725f27daa1091eedb379
https://doi.org/10.3847/1538-4357/aabad4
https://doi.org/10.3847/1538-4357/aabad4
Autor:
Terry G. Forbes, Daniel B. Seaton
Publikováno v:
The Astrophysical Journal. 701:348-359
We develop a model that predicts the velocity, density, and temperature of coronal reconnection jets in the presence of thermal conduction. Our model is based on the quasi-one-dimensional treatment of reconnecting current sheets developed by B. Somov
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::34a2be6d7d3b7b87b170f785601c8827
https://doi.org/10.1088/0004-637x/701/1/348
https://doi.org/10.1088/0004-637x/701/1/348
Publikováno v:
The Astrophysical Journal. 675:868-874
The X-Ray Telescope on Hinode has observed individual loops of plasma moving downward in a manner that is consistent with field line shrinkage in the aftermath of reconnection at higher altitudes. An on-disk B3.8 flare observed on 2007 May 2 has loop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::319bddefe6e662906d8a219abce1ac60
https://doi.org/10.1086/526336
https://doi.org/10.1086/526336