Results 21 to 30 of about 961,519 (212)

Turbulence in the Solar Photosphere [PDF]

open access: yesSpace Science Reviews, 2001
16 pages, 1 ...
openaire   +2 more sources

The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes

open access: yesThe Astrophysical Journal, 2023
Observations show that there are twisted magnetic flux tubes and plasma flow throughout the solar atmosphere. The main purpose of this work is to obtain the damping rate of sausage modes in the presence of magnetic twist and plasma flow.
Mohammad Sadeghi   +2 more
doaj   +1 more source

Current sheets in the solar corona : formation, fragmentation and heating [PDF]

open access: yes, 2011
In this thesis we investigate current sheets in the solar corona. The well known 1D model for the tearing mode instability is presented, before progressing to 2D where we introduce a non-uniform resistivity.
Bowness, Ruth
core   +2 more sources

Investigating Alfvénic wave propagation in coronal open-field regions [PDF]

open access: yes, 2015
The physical mechanisms behind accelerating solar and stellar winds are a long-standing astrophysical mystery, although recent breakthroughs have come from models invoking the turbulent dissipation of Alfvén waves.
Morton, Richard   +2 more
core   +1 more source

Latitudinal Variation of the Solar Photospheric Intensity [PDF]

open access: yesThe Astrophysical Journal, 2008
24 pages, 8 figs, accepted in ...
Rast, Mark P.   +2 more
openaire   +2 more sources

The investigation of quasi-separatrix layers in solar magnetic fields [PDF]

open access: yes, 2011
The structure of the magnetic field is often an important factor in many energetic processes in the solar corona. To determine the topology of the magnetic field features such as null points, separatrix surfaces, and separators must be found.
Restante, Anna Lisa
core   +2 more sources

Inferring depth-dependent plasma motions from surface observations using the DeepVel neural network

open access: yesJournal of Space Weather and Space Climate, 2021
Coverage of plasma motions is limited to the line-of-sight component at the Sun’s surface. Multiple tracking and inversion methods were developed to infer the transverse motions from observational data.
Tremblay Benoit   +4 more
doaj   +1 more source

Models of the Solar Photosphere [PDF]

open access: yesSymposium - International Astronomical Union, 1990
This review summarizes the main properties of the available theoretical models of the solar photosphere and the semiempirical models based primarily on observed spectra in different wavelength regions. LTE and non-LTE semiempirical models are compared with LTE and non-LTE theoretical (radiative equilibrium) models calculated with and without convective
openaire   +1 more source

STOCHASTIC COUPLING OF SOLAR PHOTOSPHERE AND CORONA [PDF]

open access: yesThe Astrophysical Journal, 2013
36 pageS, 11 figures, 3 ...
Uritsky, Vadim M.   +3 more
openaire   +2 more sources

Investigation of Phase Shift and Travel Time of Acoustic Waves in the Lower Solar Atmosphere Using Multiheight Velocities

open access: yesThe Astrophysical Journal
We report and discuss the phase shift and phase travel time of low-frequency ( ν < 5.0 mHz) acoustic waves estimated within the photosphere and photosphere–chromosphere interface regions, utilizing multiheight velocities in the quiet Sun.
Hirdesh Kumar   +4 more
doaj   +1 more source

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