Zobrazeno 1 - 10
of 96
pro vyhledávání: '"B C, Low"'
Autor:
B. C. Low
Publikováno v:
Physics of Plasmas. 30:012903
The two-plate initial boundary-value problem of Parker is reviewed, treating the relaxation of a 3D magnetic field prescribed with an arbitrary topology to a terminal force-free field in a cold, viscous, electrically perfect fluid conductor. Anchored
Autor:
B. C. Low
In the 60 years after E. N. Parker's prediction of the existence of the solar wind and the magnetic origin of coronal heating, space-borne and ground-based observations have built a conceptually complete phenomenology of the corona as a fully ionized
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3235c182681bfa176371b8475d53228e
https://doi.org/10.1016/b978-0-12-814334-6.00008-x
https://doi.org/10.1016/b978-0-12-814334-6.00008-x
Publikováno v:
Proceedings of the International Astronomical Union. 8:235-238
An enormous solar tornado was observed by SDO/AIA on 25 September 2011. It was mainly associated with a quiescent prominence with an overlying coronal cavity. We investigate the triggering mechanism of the solar tornado by using the data from two ins
Autor:
B. C. Low, Å. M. Janse
Publikováno v:
Astronomy & Astrophysics. 472:957-965
Aims. The released magnetic energy in coronal events, i.e. in flares and coronal mass ejections (CMEs), is believed to have been stored locally in the coronal magnetic field. The energy in a magnetic field B is distributed in space with density B 2 8
Autor:
Gordon Petrie, B. C. Low
Publikováno v:
The Astrophysical Journal Supplement Series. 159:288-313
The solar corona is continually being injected with magnetic flux from the solar interior, flux that cannot be annihilated in bulk by the electrically highly conducting corona. Observations have shown that mass loss through downflows within solar pro
Autor:
Sarah Gibson, B. C. Low
Publikováno v:
Journal of Geophysical Research: Space Physics. 105:18187-18202
A physical interpretation of observed coronal “on-disk” manifestations of an Earth-directed coronal mass ejection (CME) is presented. The fundamental question of how the CME's magnetic field and its plasma distribution are related is largely unan
Autor:
B. C. Low, Ward B. Manchester
Publikováno v:
Physics of Plasmas. 7:1263-1279
A physical analysis is presented of two distinct families of two-dimensional (2D) analytical solutions for isothermal periodic magnetostatic atmospheres in uniform gravity, one arrived at by Dungey and the other arrived at by Low and Manchester. It i
Publikováno v:
Physics of Plasmas. 6:954-969
A simple, compact, and systematic derivation is given of the characteristic properties of the magnetohydrodynamic (MHD) equations with two independent variables (time-dependent MHD in the xt plane and steady MHD in the xy plane), based on the symmetr
Publikováno v:
Physics of Plasmas. 5:4015-4027
Two-dimensional ideal magnetohydrodynamic (MHD) simulations are presented that demonstrate several novel phenomena in MHD shock formation. The stationary symmetrical flow of a uniform, planar, field-aligned, low-β and superfast magnetized plasma aro
Autor:
B. C. Low
Publikováno v:
Solar System Plasma Physics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9c30bab0ae8b337d8c5f569dffb20033
https://doi.org/10.1029/gm054p0021
https://doi.org/10.1029/gm054p0021