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Analysis of temporal variations of dynamic textures by means of the SGLDM with application to EIT solar images

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Języki publikacji
EN
Abstrakty
EN
The paper discusses applicability of texture analysis methods to Extreme-Ultraviolet Imaging Telescope (EIT) images obtained from the SOHO mission, and in particular analyses of the solar texture by means of the Spatial Gray Level Dependence Matrices (SGLDMs). Based on the observations, a theoretical parametric model is proposed for the SGLDM. Subsequently, the Haralick features are computed directly for the time sequence of preprocessed images, as well as and for the proposed model of the SGLDM. Time evolution of model parameters as well as measures of goodness fit of the model to image data for the period of one year is presented. The results obtained confirm the correctness of the model. In view of the simplicity of the model, it gives remarkably good results. A new method for solar limb extraction is described in the Appendix. The method is superior to those presented in the literature since it uses no external parameters, such as thresholds.
Słowa kluczowe
Rocznik
Strony
219--247
Opis fizyczny
Bibliogr. 26 poz., rys., tab., wykr.
Twórcy
autor
  • Institute of Fundamental Technological Research, Polish Academy of Sciences, ul. Swietokrzyska 21, 00-049 Warsaw, Poland, kbojar@ippt.gov.pl
Bibliografia
  • [1] Haralick R., Shanmugam K., Dinstein I.: Textural features for image classification. IEEE Trans. Systems, Man And Ctbern., 3(6), 610-621, 1973
  • [2] Bray J., Loughhead R., Durrant C.: The solar granulation. Cambridge University Press, London, 1984.
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  • [6] Delaboudiniere J., Artzner G., et al.: EIT: Extreme-ultraviolet Imaging Telescope: for the SOHO mission. Solar Phys., 162, 291-312, 1996.
  • [7] Pauluhn A., Solanki S., Rüedi I., Schühle U.: Statistics of quiet sun extreme ultraviolet intensities. Astron. & Astrophys., 362, 737-7415, 2000.
  • [8] Hochedez, J-F., Clette F., Verwichte E., Berghmans D., Cugnon P.: Mid-terrn variations in the extreme UV corona: the EIT/SOHO perspective. ESA SP, 463, 79-85, 2000.
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  • [10] Roerdink J.: Group morphology. Pat. Rec., 33, 877-895, 2000.
  • [11] Hochedez J-F., Clette F., Verwichte E., Berghmans D., Cugnon P.: Long term variations in the extreme UV corona: the EIT/SOHO perspective. Adv. in Soft Comp. Conf. Series, 200, 501-504, 2001.
  • [12] Canfield R. C.: Solar active regions. In: Murdin P. (Ed.) Encyclopedia of Astronomy and Astrophysics, Vol. 3, 2457-2462. Institute of Physics Publishing, Bristol, 2001.
  • [13] Cranmer S. R.: Coronal holes. In: Murdin P. (Ed.) Encyclopedia of Astronomy and Astrophysics, Vol. 1, 496-501. Institute of Physics Publishing, Bristol, 2001.
  • [14] Portier-Fozzani F., Vandame B., Bijaoui A., Maucherat A. J., EIT Team: A multiscale vision model applied to analyze EIT images of the solar corona. Solar Phys., 201(2), 271-288, 2001.
  • [15] Hochedez J-F., Jacques L., Verwichte E., Berghmans D., Wauters L., Clette F., Cugnon P.: Multiscale activity observed by EIT/SOHO. ESA SP, 477, 115-118, 2002.
  • [16] Hochedez J-F., Jacques L., Zhukov A., Clette F., Antoine J-P.: Small features in the EIT-SOHO images. ESA SP, 508 295-298, 2002.
  • [17] Brajsa R., Wéhl H., Vrsnak B., Ruzdjak V., Clette F., Hochedez J-F.: Solar differential rotation determined by tracing coronal bright points in SOHO/EIT images. Astron. & Astrophys., 392, 329: 334, 2002.
  • [18] Gontikakis C., Peter H., Dara H.: Sizes of quiet sun transition region structures. Astron. & Astrophys., 408, 743-753, 2003.
  • [19] Zharkova V., Ipson S., Zharkov S., Benkhalil A., Abourdarham J., Bentley R.: A full-disk image standarisation of the synoptic solar observations at the Meudon Observatory. Solar Phys., 214(l), 89-105, 2003.
  • [20] Ravindra B., Venkatakrishnan P.: Structure and evolution of the transition region network observed in He II 304. Solar Phys., 215, 239-259, 2003.
  • [21] Pluim J., Maintz J., Viergever M.: Mutual-information-based registration of medical images: a survey. IEEE Trans. Med. Imag., 22(10), 986-1004, 2003.
  • [22] De Groof A., Berghmans D., van Driel-Gesztelyi L., Poedts S.: Intensity variations in EIT shutterless L mode: Waves or flows. Astron. & Astrophys., 415, 1141-1151, 2004.
  • [23] Del Moro D.: Solar granulation properties derived from three different time series. Astron. & Astrophys., 428, 1007-1015, 2005.
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  • [25] Chetverikov D., Péteri R.: A brief survey of dynamic texture description and recognition.
  • [26] Bojar K., Nieniewski M.: Modelling the spectrum of the Fourier transform of the texture in the solar EIT images. Machine Graphics & Vision, in press, 2006.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-article-BWA1-0036-0001
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