Quantifying Spicules

@inproceedings{Pereira2012QuantifyingS,
  title={Quantifying Spicules},
  author={T. Pereira and B. Pontieu and M. Carlsson},
  year={2012}
}
Understanding the dynamic solar chromosphere is fundamental in solar physics. Spicules are an important feature of the chromosphere, connecting the photosphere to the corona, potentially mediating the transfer of energy and mass. The aim of this work is to study the properties of spicules over different regions of the sun. Our goal is to investigate if there is more than one type of spicules, and how spicules behave in the quiet sun, coronal holes, and active regions. We make use of high… Expand
ON THE TEMPORAL EVOLUTION OF SPICULES OBSERVED WITH IRIS, SDO, AND HINODE
On the multi-threaded nature of solar spicules
An Interface Region Imaging Spectrograph First View on Solar Spicules
High--cadence observations of spicular-type events on the Sun
Macrospicules, jets and the solar chromosphere
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References

Society of Photo-Optical Instrumentation Engineers