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Solar and Heliospheric Physics with the Square Kilometre Array View all abstracts by submitter

Valery Nakariakov   Submitted: 2014-12-23 05:09

The fields of solar radiophysics and solar system radio physics, or radio heliophysics, will benefit immensely from an instrument with the capabilities projected for SKA. Potential applications include interplanetary scintillation (IPS), radio-burst tracking, and solar spectral radio imaging with a superior sensitivity. These will provide breakthrough new insights and results in topics of fundamental importance, such as the physics of impulsive energy releases, magnetohydrodynamic oscillations and turbulence, the dynamics of post-eruptive processes, energetic particle acceleration, the structure of the solar wind and the development and evolution of solar wind transients at distances up to and beyond the orbit of the Earth. The combination of the high spectral, time and spatial resolution and the unprecedented sensitivity of the SKA will radically advance our understanding of basic physical processes operating in solar and heliospheric plasmas and provide a solid foundation for the forecasting of space weather events.

Authors: Valery M. Nakariakov, Mario M. Bisi, Philippa K. Browning, Dalmiro Maia, Eduard P. Kontar, Divya Oberoi, Peter T. Gallagher, Iver H. Cairns, Heather Ratcliffe
Projects: None

Publication Status: Proc. of Science (in press), 2015
Last Modified: 2014-12-23 14:49
Go to main E-Print page  The process of data formation for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar Orbiter  Coronal turbulence and the angular broadening of radio sources - the role of the structure function  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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