Contribution of polar plumes to fast solar wind

@article{Zangrilli2020ContributionOP,
  title={Contribution of polar plumes to fast solar wind},
  author={Luca Zangrilli and Sezione di Torino and Pino Torinese and Italy.},
  journal={Astronomy and Astrophysics},
  year={2020},
  volume={643}
}
Context. Several physical properties of solar polar plumes have been identified by different published studies, however such studies are rare and sometimes in disagreement. Aims. The purpose of the present work is to analyze a set of SOHO/UVCS data dedicated to the observation of plumes and to obtain a picture of the physical properties of plumes in the intermediate solar corona through a self-consistent analysis. Methods. We applied the Doppler Dimming technique to data acquired by SOHO/UVCS… 
Population of Bright Plume Threads in Solar Polar Coronal Holes
Coronal holes are well accepted to be source regions of the fast solar wind. As one of the common structures in coronal holes, coronal plumes might contribute to the origin of the nascent solar wind.
On the Nature of Propagating Intensity Disturbances in Polar Plumes during the 2017 Total Solar Eclipse
The propagating intensity disturbances (PIDs) in plumes are still poorly understood, and their identity (magnetoacoustic waves or flows) remains an open question. We investigate PIDs in five plumes

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