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Analysis of full-disc Ca II K spectroheliograms: III. Plage area composite series covering 1892-2019

Authors :
European Commission
Ministry of Education (South Korea)
Chatzistergos, Theodosios
Ermolli, Ilaria
Krivova, Natalie A.
Solanki, Sami K.
Banerjee, Dipankar
Barata, Teresa
Belik, Marcel
Gafeira, Ricardo
Garcia, Adriana
Hanaoka, Yoichiro
Hegde, Manjunath
Klimeš, Jan
Korokhin, Viktor V.
Lourenço, Ana
Malherbe, Jean-Marie
Marchenko, Gennady P.
Peixinho, Nuno
Sakurai, Takashi
Tlatov, Andrey G.
European Commission
Ministry of Education (South Korea)
Chatzistergos, Theodosios
Ermolli, Ilaria
Krivova, Natalie A.
Solanki, Sami K.
Banerjee, Dipankar
Barata, Teresa
Belik, Marcel
Gafeira, Ricardo
Garcia, Adriana
Hanaoka, Yoichiro
Hegde, Manjunath
Klimeš, Jan
Korokhin, Viktor V.
Lourenço, Ana
Malherbe, Jean-Marie
Marchenko, Gennady P.
Peixinho, Nuno
Sakurai, Takashi
Tlatov, Andrey G.
Publication Year :
2020

Abstract

Context. Studies of long-term solar activity and variability require knowledge of the past evolution of the solar surface magnetism. The archives of full-disc Ca II K observations that have been performed more or less regularly at various sites since 1892 can serve as an important source of such information. Aims. We derive the plage area evolution over the last 12 solar cycles by employing data from all Ca II K archives that are publicly available in digital form, including several as-yet-unexplored Ca II K archives. Methods. We analysed more than 290 000 full-disc Ca II K observations from 43 datasets spanning the period between 1892-2019. All images were consistently processed with an automatic procedure that performs the photometric calibration (if needed) and the limb-darkening compensation. The processing also accounts for artefacts affecting many of the images, including some very specific artefacts, such as bright arcs found in Kyoto and Yerkes data. Our employed methods have previously been tested and evaluated on synthetic data and found to be more accurate than other methods used in the literature to treat a subset of the data analysed here. Results. We produced a plage area time-series from each analysed dataset. We found that the differences between the plage areas derived from individual archives are mainly due to the differences in the central wavelength and the bandpass used to acquire the data at the various sites. We empirically cross-calibrated and combined the results obtained from each dataset to produce a composite series of plage areas. The 'backbone' approach was used to bridge the series together. We have also shown that the selection of the backbone series has little effect on the final composite of the plage area. We quantified the uncertainty of determining the plage areas with our processing due to shifts in the central wavelength and found it to be less than 0.01 in fraction of the solar disc for the average conditions found on historic

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1286553628
Document Type :
Electronic Resource