Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-11T06:58:56.577Z Has data issue: false hasContentIssue false
  • English
  • Français

Solar Radio Emission as a Prediction Technique for Coronal Mass Ejections’ Detection

Published online by Cambridge University Press:  24 July 2018

Vladimir M. Fridman  and
Olga A. Sheiner Open the ORCID record for Olga A. Sheiner [Opens in a new window]
Vladimir M. Fridman
Affiliation:
Radiophysical Research Institute, National Lobachevsky State University, 25/12A Bol’shaya Pecherskaya str., 603950, Nizhny Novgorod, Russian Federation email: rfj@nirfi.unn.ru
Olga A. Sheiner
Affiliation:
Radiophysical Research Institute, National Lobachevsky State University, 25/12A Bol’shaya Pecherskaya str., 603950, Nizhny Novgorod, Russian Federation email: rfj@nirfi.unn.ru
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this report we present a possible scheme of short-term CME detection forecasting developed on the basis of statistical analysis of solar radio emission regularities prior to “isolated” solar Coronal Mass Ejections registered in 1998, 2003, 2009-2013.

Keywords

Sun: radio radiationSun: coronal mass ejections (CMEs)methods: data analysis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S335: Space Weather of the Heliosphere: Processes and Forecasts , July 2017 , pp. 321 - 323
Copyright
Copyright © International Astronomical Union 2018 

References

Fridman, V. M. & Sheiner, O. A. 2009, Geomagnetism & Aeronomy, 49, 1133Google Scholar
Sheiner, O. A. & Durasova, M. S. 1994, Radiophysics & Quantum Electronics, 37, 575Google Scholar
Sheiner, O. A. & Fridman, V. M. 2010, Radiophysics & Quantum Electronics, 53, 281Google Scholar