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Statements

Subject Item
n2:RIV%2F00216305%3A26210%2F06%3APU64165%21RIV07-MSM-26210___
rdf:type
n15:Vysledek skos:Concept
dcterms:description
A new numerical method of image processing suitable for visualization of corona images taken during total solar eclipses is presented. The method is based on the use of adaptive filters inspired by human vision and the sensitivity of resulting images is very close to that of the human eye during an eclipse. This method highly improves a widely used unsharp masking method employing a radially blurred mask. A high precision alignment method for white light corona images is also discussed. The results of these numerical image processing techniques are illustrated by images obtained by expeditions to observe total solar eclipses organized by the Astronomical Institute of the Slovak Academy of Sciences, Upice Observatory and Miloslav Druckmüller. A new numerical method of image processing suitable for visualization of corona images taken during total solar eclipses is presented. The method is based on the use of adaptive filters inspired by human vision and the sensitivity of resulting images is very close to that of the human eye during an eclipse. This method highly improves a widely used unsharp masking method employing a radially blurred mask. A high precision alignment method for white light corona images is also discussed. The results of these numerical image processing techniques are illustrated by images obtained by expeditions to observe total solar eclipses organized by the Astronomical Institute of the Slovak Academy of Sciences, Upice Observatory and Miloslav Druckmüller. A new numerical method of image processing suitable for visualization of corona images taken during total solar eclipses is presented. The method is based on the use of adaptive filters inspired by human vision and the sensitivity of resulting images is very close to that of the human eye during an eclipse. This method highly improves a widely used unsharp masking method employing a radially blurred mask. A high precision alignment method for white light corona images is also discussed. The results of these numerical image processing techniques are illustrated by images obtained by expeditions to observe total solar eclipses organized by the Astronomical Institute of the Slovak Academy of Sciences, Upice Observatory and Miloslav Druckmüller.
dcterms:title
A new numerical method of total solar eclipse photography processing A new numerical method of total solar eclipse photography processing A new numerical method of total solar eclipse photography processing
skos:prefLabel
A new numerical method of total solar eclipse photography processing A new numerical method of total solar eclipse photography processing A new numerical method of total solar eclipse photography processing
skos:notation
RIV/00216305:26210/06:PU64165!RIV07-MSM-26210___
n3:strany
131-147
n3:aktivita
n14:S
n3:aktivity
S
n3:cisloPeriodika
3
n3:dodaniDat
n4:2007
n3:domaciTvurceVysledku
n7:8961905
n3:druhVysledku
n10:J
n3:duvernostUdaju
n8:S
n3:entitaPredkladatele
n16:predkladatel
n3:idSjednocenehoVysledku
463659
n3:idVysledku
RIV/00216305:26210/06:PU64165
n3:jazykVysledku
n17:eng
n3:klicovaSlova
solar eclipse, image processing, adaptive filter
n3:klicoveSlovo
n6:solar%20eclipse n6:adaptive%20filter n6:image%20processing
n3:kodStatuVydavatele
SK - Slovenská republika
n3:kontrolniKodProRIV
[6B46050499D0]
n3:nazevZdroje
Contributions of the Astronomical Observatory Skalnaté Pleso
n3:obor
n12:BL
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
3
n3:rokUplatneniVysledku
n4:2006
n3:svazekPeriodika
2006
n3:tvurceVysledku
Druckmüller, Miloslav Minarovjech, Milan Rušin, Vojtěch
s:issn
1335-1842
s:numberOfPages
17
n13:organizacniJednotka
26210