MODULATIONAL INSTABILITY OF THE RADIAL VIBRATIONS OF CORONAL LOOPS
https://doi.org/10.33236/2307-910Х-2018-4-24-212-215
Abstract
Axisymmetric modes in coronal loops are used to interpret observed fast microwave and hard x-ray pulsations. Their properties are well studied in the approximation of linear magnetic hydrodynamics. Currently, axisymmetric modes of large amplitude are actively investigated.
About the Authors
Galina Alekseevna Mankaeva
Kalmyk state University
Russian Federation
Russian Federation
Naga Varoon Yealagandula
Kalmyk state University
Russian Federation
Russian Federation
Badma Borisovich Mikhalyaev
Kalmyk state University
Russian Federation
Russian Federation
Lyudmila Naranova Dzhimbeyeva
Kalmyk state University
Russian Federation
Russian Federation
References
1. Nakariakov V. М., Melnikov V. F. 2009. Space Sci. Rev. 149, 119.
2. Inglies 2008. Astron. Astrophys. 487, 1147.
3. Huang 2014. Astrophys. J. 791, A44.
4. Mikhalyaev В. В., Ruderman M. S. 2015. J. Plasma Phys. 81, 905810611.
5. Mikhalyaev В. В., Ruderman M. S., Naga Varan E. 2016. Geomagnetism and Aeronomy. 56, 1040-1044.
Review
For citations:
Mankaeva G.A., Yealagandula N.V., Mikhalyaev B.B., Dzhimbeyeva L.N. MODULATIONAL INSTABILITY OF THE RADIAL VIBRATIONS OF CORONAL LOOPS. Modern Science and Innovations. 2018;(4):212-215. (In Russ.) https://doi.org/10.33236/2307-910Х-2018-4-24-212-215
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