The effect of plume/interplume lanes on ion-cyclotron resonance heating

Details The effect of plume/interplume lanes on ion-cyclotron resonance heating The effect of plume/interplume lanes on ion-cyclotron resonance heating

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..274..137d&link_type=abstract

Advances in Plasma Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 274, p. 137-139

Astronomy and Astrophysics

Astrophysics

Sun: Corona, Solar Wind, Acceleration Of Particles, Plasmas, Waves

Scientific paper

The effect of the Plume/Interplume Lane (PIPL) structure of the solar
North Polar Coronal Hole (NPCH) on the ion-cyclotron resonance (ICR)
process is investigated. The ICR process in the interplume lanes is much
more effective than in the plumes, agreeing with the observations which
show the source of fast solar wind is interplume lanes.

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