Indirect comparison of Debrecen and Greenwich daily sums of sunspot areas
arXiv:1306.5621 · doi:10.1093/mnras/stt1134
Abstract
Sunspot area data play an important role in the studies of solar activity and its long-term variations. In order to reveal real long-term solar variations precise homogeneous sunspot area databases should be used. However, the measured areas may be burdened with systematic deviations, which may vary in time. Thus, there is a need to investigate the long-term variation of sunspot area datasets and to determine the time-dependent cross-calibration factors. In this study, we investigate the time-dependent differences between the available long-term sunspot databases. Using the results, we estimate the correction factor to calibrate the corrected daily sunspot areas of Debrecen Photoheliographic Data (DPD) to the same data of Greenwich Photoheliographic Results (GPR) by using the overlapping Kislovodsk and Pulkovo data. We give the correction factor as GPR=1.08(\pm 0.11)*DPD
9 pages, 7 figures, Accepted for publication in MNRAS
References in corpus (1)
Cited by in corpus (11)
- On-line Tools for Solar Data Compiled at the Debrecen Observatory and their Extensions with the Greenwich Sunspot Data
- Sunspot area catalogue revisited: Daily cross-calibrated areas since 1874
- Comparative analysis of Debrecen sunspot catalogues
- Solar cycle indices from the photosphere to the corona: measurements and underlying physics
- Different contributions to space weather and space climate from different big solar active regions
- Extending the Sunspot Area Series from Kodaikanal Solar Observatory
- Dark dots on the photosphere and counting of the sunspots index
- On the size distribution of spots within sunspot groups
- An alternative measure of solar activity from detailed sunspot datasets
- Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods
- Comparison of automatic methods to detect sunspots in the Coimbra Observatory spectroheliograms