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Browsing by Subject "Coronal loops"

Browsing by Subject "Coronal loops"

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  • Coronal Loops 
    Krishan, V (Indian Institute of Astrophysics, Bangalore, 1986)
    The statistical treatment of the magnetohydrodynamically turbulent plasma is used to study the steady state configuration of the coronal loops. The stability of the plasma system is defined in terms of certain invariants ...
  • Equilibrium of a thin, isolated, axisymmetric force-free magnetic flux tube in a stratified atmosphere 
    Lakshmi, P; Gokhale, M. H (Kluwer Academic Publishers, 1988-03)
    The equations for equilibrium of a thin, isolated, axisymmetric, and force-free magnetic flux tube are derived, taking into account the inhomogeneities of the magnetic field, plasma pressure, and plasma density over the ...
  • Filament activity in a quiet region flare 
    Sundararaman, K; Gupta, S. S; Selvendran, R (Indian Academy of Sciences, 1993-03)
    We have taken the case of a circular H-alpha filament observed on May 9, 1979 erupting into a double-ribbon flare associated with a nonspot region. The plage motions are responsible for the filament reorientation and, here ...
  • Global sausage and kink modes in coronal loops 
    Anasooya Ashok; Satya Narayanan, A; Ramesh, R; Kathiravan, C (Anita Publications, 2004)
  • Magnetic Helicity of Oscillating Coronal Loops 
    Krishan, V; Priest, E. R (International Astronomical Union, 1990)
  • VLA observations of solar active regions at 6 and 20 CM 
    Alissandrakis, C. E; Kundu, M. R; Shevgaonkar, R. K (The European Southern Observatory, 1991-11)
    High-resolution observations are presented of two active regions at 6 and 20 cm over a period of 5 days, together with H-alpha and photospheric magnetic fields. The large-scale emission at 20 cm is associated with the ...
  • Vlasov-Maxwell equilibria of solar coronal loops 
    Krishan, V; Sreedharan, T. D; Mahajan, Swadesh M (Royal Astronomical Society, 1991-04)
    A Vlasov-Maxwell description of the ubiquitous solar coronal structures is presented. It is found that an equilibrium plasma configuration can live with spatial gradients in density, temperature, current and drift speeds ...

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