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 language | English |
|---|---|
| Pages (from-to) | 449-460 |
| Number of pages | 11 |
| Journal | Solar Physics |
| Volume | 262 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - Apr 2010 |
Keywords
- corona
- prominences
- solar physics
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Automatic detection of limb prominences in 304 A EUV images
Labrosse, N., Dalla, S., Marshall, S. & Gray, N., 23 Apr 2009.Research output: Contribution to conference › Paper
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