Chromospheric Evaporation in Solar Flares

  • Zongjun Ning
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 30)


Chromospheric evaporation implies the mass flow from chromosphere to corona along the loop legs in the solar flares. From observations, radio emissions show the high-frequency cutoff and with a drift toward the low frequency, and the coronal lines display a strong blueshift on the Doppler diagram, and hard X-ray emissions tend to rise up the double footpoint sources along the loop legs and finally merge together around the top at the same position as the loop top source. In this paper, we briefly review the radio, EUV and X-ray evidences of the chromospheric evaporation from the documents in recent years.


Radio Emission Drift Rate Solar Energetic Particle Event Flare Ribbon Chromospheric Evaporation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.



This work is supported by NSF of China under grants 10833007, 40804034, 10973042, 973 Program under grant 2011CB811400 and Laboratory No. 2010DP173032.


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Copyright information

© Springer-Verlag Berlin Heidelberg 2012

Authors and Affiliations

  1. 1.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain ObservatoryNanjingChina

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