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Pregled bibliografske jedinice broj: 910108

Determination of the Kanzelhoehe sunspot group positions: manual versus automatic method


Poljančić Beljan, Ivana; Jurdana - Šepić, Rajka; Brajša, Roman; Hržina, Damir; Poetzi, Werner; Hanslmeier, Arnold; Ruždjak, Domagoj; Sudar, Davor; Skokić, Ivica; Woehl, Hubertus
Determination of the Kanzelhoehe sunspot group positions: manual versus automatic method // Multi-Wavelength Studies of the Solar Atmosphere: Celebrating the Career of Costas Alissandrakis
Ioannina, Grčka, 2015. (predavanje, nije recenziran, neobjavljeni rad, znanstveni)


Naslov
Determination of the Kanzelhoehe sunspot group positions: manual versus automatic method

Autori
Poljančić Beljan, Ivana ; Jurdana - Šepić, Rajka ; Brajša, Roman ; Hržina, Damir ; Poetzi, Werner ; Hanslmeier, Arnold ; Ruždjak, Domagoj ; Sudar, Davor ; Skokić, Ivica ; Woehl, Hubertus

Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, neobjavljeni rad, znanstveni

Skup
Multi-Wavelength Studies of the Solar Atmosphere: Celebrating the Career of Costas Alissandrakis

Mjesto i datum
Ioannina, Grčka, 21-24.9.2015

Vrsta sudjelovanja
Predavanje

Vrsta recenzije
Nije recenziran

Ključne riječi
Sunspot groups positions, differential rotation, differential rotation coefficients

Sažetak
For the investigation of possible variations of the solar rotation, sunspots and sunspot groups are very often used as tracers, mainly because of the long term data sets available from various observatories. Until now, for the investigation of temporal variations of the solar rotation using sunspot groups as tracers, the Kanzelhoehe data set was analysed only for the period 1947-1981. Our aim is to provide a continuation of that previous investigation. For this reason we processed Kanzelhoehe sunspot drawings for solar cycles nos. 20-23 (manual method) and Kanzelhoehe white light images for solar cycle no. 24 (automatic method), covering almost the 41 year period, 1964 - 2015. When both methods for the heliographic positions determination have been used, it is important to compare them. Here we present the results of the manual versus automatic method comparison (differential rotation coefficients for both methods, differences in the identi cation of the sunspot groups, differences in the number of identi fied sunspot groups, etc.) performed for the year 2014.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Ustanove
Geodetski fakultet, Zagreb,
Sveučilište u Rijeci - Odjel za fiziku