首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Increasing the Fine Structure Visibility of the Hinode SOT Ca ii H Filtergrams
Authors:E Tavabi  S Koutchmy  A Ajabshirizadeh
Institution:1. Physics Department, Payame Noor University, 19395-3697, Tehran, I. R. of Iran
2. UMR 7095, CNRS & UPMC, Institut d’Astrophysique de Paris, 98 Bis Bd Arago, 75014, Paris, France
3. Center for Excellence in Astronomy & Astrophysics (CEAA – RIAAM), P.O. Box 55134 – 441, Maragha, Iran
Abstract:We present an image processing technique, the improved OMC filter (also called Madmax), which selects maxima of convexities of intensity modulations of an image. The filter computes second derivatives of the image in multiple directions around each pixel. It is shown to be efficient for pattern recognition, and bright hair-like or small anisotropic features can be enhanced. The filter is tested on artificially generated images, and the effect of a different number of directions in which the second derivatives are calculated is evaluated. Ca ii H line images of spicules and prominences obtained with Hinode/SOT are also used to illustrate its efficiency on real data. It is shown how to make the choice of the sensitive parameters to be used in improving the image visibility.
Keywords:
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号