Results 111 to 120 of about 12,081 (211)

The origin and dynamic interaction of solar magnetic fields [PDF]

, 2007
The dynamics of the solar corona are dominated by the magnetic field which creates its structure. The magnetic field in most of the corona is ‘frozen’ to the plasma very effectively.
Antonia Wilmot-Smith, Wilmot-Smith, Antonia, Wilmot-Smith, A.L.   +2 more
core  

The influence of Hall currents, plasma viscosity and electron inertia on magnetic reconnection solutions

, 2007
This thesis examines magnetic reconnection in the solar corona. Magnetic reconnection is the only mechanism which allows the magnetic topology of magnetized plasmas to be changed. Many of the dynamic processes in the Sun's atmosphere are believed to be
Senanayake, Tissa
core  

Comprehensive Synthesis of Magnetic Tornado: Cospatial Incidence of Chromospheric Swirls and Extreme-ultraviolet Brightening

The Astrophysical Journal Letters
Magnetic tornadoes, characterized as impulsive Alfvén waves initiated by photospheric vortices in intergranular lanes, are considered efficient energy channels to the corona.
Hidetaka Kuniyoshi, Souvik Bose, Takaaki Yokoyama   +2 more
doaj   +1 more source

Magnetohydrodynamic waves in structured atmospheres

, 2012
The effect of structuring, in the form of magnetic or density inhomogeneities, on the magnetohydrodynamic (mhd) waves of an infinite plasma is investigated.
Edwin, Patricia Mary
core  

Relevant heating of the quiet solar corona by Alfvén waves: a result of adiabaticity breakdown. [PDF]

Sci Rep, 2019
Escande DF, Gondret V, Sattin F.
europepmc   +1 more source

Solar Wind Acceleration from the Upper Chromosphere to the Corona in Coronal Hole Regions

, 1999
Flow speeds derived in recent years from chromospheric/transition region and coronal observations suggest that the solar wind acceleration process might start at heights in the solar atmosphere much lower than previously imagined.
Esser, Ruth
core  

Evidence for small-scale torsional Alfvén waves in the solar corona. [PDF]

Nat Astron
Morton RJ, Gao Y, Tajfirouze E, Tian H, Van Doorsselaere T, Schad TA.   +5 more
europepmc   +1 more source

On Field Line Slippage Rates in the Solar Corona. [PDF]

Sol Phys
MacTaggart D.
europepmc   +1 more source

Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona. [PDF]

Nat Commun, 2019
Carley EP, Hayes LA, Murray SA, Morosan DE, Shelley W, Vilmer N, Gallagher PT.   +6 more
europepmc   +1 more source

Magnetoacoustic wave propagation in the solar corona and filament dynamics. [PDF]

Sci Rep
Somaiyeh S, Stefaan P.
europepmc   +1 more source