Automatic detection of limb prominences in 304 A EUV images

N. Labrosse, S. Dalla, S. Marshall, N. Gray

Research output: Contribution to conferencePaper

Abstract

A new algorithm for automatic detection of prominences on the solar limb in 304 Å EUV images is presented, and results of its application to SOHO/EIT data discussed. The detection is based on the method of moments combined with a classifier analysis aimed at discriminating between limb prominences, active regions, and the quiet corona. This classifier analysis is based on a Support Vector Machine (SVM). Using a set of 12 moments of the radial intensity profiles, the algorithm performs well in discriminating between the above three categories of limb structures, with a misclassification rate of 7%. Pixels detected as belonging to a prominence are then used as the starting point to reconstruct the whole prominence by morphological image-processing techniques. It is planned that a catalogue of limb prominences identified in SOHO and STEREO data using this method will be made publicly available to the scientific community.
Original languageEnglish
Publication statusUnpublished - Apr 2009
EventRAS National Astronomy Meeting 2009 - London, UK
Duration: 19 Apr 200924 Apr 2009

Conference

ConferenceRAS National Astronomy Meeting 2009
CityLondon, UK
Period19/04/0924/04/09

Keywords

  • corona
  • prominences
  • solar physics
  • sun

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    Labrosse, N., Dalla, S., Marshall, S., & Gray, N. (2009). Automatic detection of limb prominences in 304 A EUV images. Paper presented at RAS National Astronomy Meeting 2009, London, UK, .