Zobrazeno 1 - 10
of 948
pro vyhledávání: '"Spheromak"'
Autor:
Bruce I. Cohen
Publikováno v:
IEEE Transactions on Plasma Science. 48:757-767
Computational plasma physics was born some 50 years ago with the development of high-speed computers. Computer simulation is well suited to the challenging nature of fundamental and applied plasma science, which exhibits enormous ranges of time and s
Publikováno v:
The Astrophysical Journal Letters
In-situ measurements carried out by spacecraft in radial alignment are critical to advance our knowledge on the evolutionary behavior of coronal mass ejections (CMEs) and their magnetic structures during propagation through interplanetary space. Yet,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e447502f35651e549d8fc84e2503b08
http://arxiv.org/abs/2106.10554
http://arxiv.org/abs/2106.10554
Autor:
Manjit Kaur, Michael R. Brown
Publikováno v:
Fusion Science and Technology. 75:275-282
Magnetothermodynamics is the study of compression and expansion of magnetized plasma with an eye toward identifying equations of state (EOSs) for magneto-inertial fusion experiments. We present recent results from Swarthmore Spheromak Experiment (SSX
Autor:
Eleanna Asvestari, Jens Pomoell, Theodosios Chatzistergos, Emilia Kilpua, Jasmina Magdalenic, Erika Palmerio, Simon Good, Stefaan Poedts, Manuela Temmer
Coronal mass ejections (CMEs) are primary drivers of space weather phenomena. Modelling the evolution of the internal magnetic field configuration of CMEs as they propagate through the interplanetary space is an essential part of space weather foreca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bffade0ca0f388d5879a64b2c8294bb8
https://doi.org/10.5194/egusphere-egu21-3291
https://doi.org/10.5194/egusphere-egu21-3291
Akademický článek
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Publikováno v:
Journal of Plasma Physics. 86
We consider the tilting instability of a magnetically confined spheromak using 3D MHD and relativistic PIC calculations with an application to astrophysical plasmas, specifically those occurring in magnetar magnetospheres. The instability is driven b
Publikováno v:
Earth, Planets and Space, Vol 73, Iss 1, Pp 1-10 (2021)
Coronal mass ejections (CMEs) cause various disturbances of the space environment; therefore, forecasting their arrival time is very important. However, forecasting accuracy is hindered by limited CME observations in interplanetary space. This study
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45d008ed68bea7fbac312c47c7ee85e0
https://doi.org/10.21203/rs.3.rs-32257/v1
https://doi.org/10.21203/rs.3.rs-32257/v1
Publikováno v:
Plasma
Volume 3
Issue 1
Pages 4-37
Volume 3
Issue 1
Pages 4-37
We describe experiments and simulations of dynamical merging with two Taylor state plasmas in a Swarthmore Spheromak Experiment (SSX) device. Taylor states are formed by magnetized plasma guns at opposite ends of the device. We performed experiments
Coronal Mass Ejections (CMEs) are one of the primary drivers of extreme space weather. They are large eruptions of mass and magnetic field from the solar corona and can travel the distance between Sun and Earth in half a day to a few days. Prediction
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f20cb1b79d9afa895ae17742641c64c1
http://arxiv.org/abs/2002.10409
http://arxiv.org/abs/2002.10409
The magnetic fields of interplanetary coronal mass ejections (ICMEs), which originate close to the Sun in the form of a flux rope, determine their geoeffectiveness. Therefore, robust flux rope-based models of CMEs are required to perform magnetohydro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c15da4b118f46cb6b577ce70804873ec
http://arxiv.org/abs/2002.10057
http://arxiv.org/abs/2002.10057