Detail publikačního výsledku

A new numerical method for solar corona image processing

DRUCKMÜLLEROVÁ, H.

Originální název

A new numerical method for solar corona image processing

Anglický název

A new numerical method for solar corona image processing

Druh

Článek recenzovaný mimo WoS a Scopus

Originální abstrakt

New variable-kernel convolution filters suitable for solar corona image processing are presented in this paper. They enable to remove an extreme gradient in radial direction and to enhance fine coronal structures without creating processing artifacts. Introduced fast algorithm enables effective computer implementation. The method is illutrated on images taken during the total solar eclipse on August 11, 1999 in Hungary.

Anglický abstrakt

New variable-kernel convolution filters suitable for solar corona image processing are presented in this paper. They enable to remove an extreme gradient in radial direction and to enhance fine coronal structures without creating processing artifacts. Introduced fast algorithm enables effective computer implementation. The method is illutrated on images taken during the total solar eclipse on August 11, 1999 in Hungary.

Klíčová slova

image processing, solar corona, eclipse

Klíčová slova v angličtině

image processing, solar corona, eclipse

Autoři

DRUCKMÜLLEROVÁ, H.

Vydáno

01.03.2005

Nakladatel

I.A.P.P.P.

Místo

USA

Svazek

2005

Číslo

99

Strany od

1

Strany do

4

Strany počet

4

BibTex

@article{BUT44078,
  author="Hana {Druckmüllerová}",
  title="A new numerical method for solar corona image processing",
  year="2005",
  volume="2005",
  number="99",
  pages="1--4"
}