Academic Journal
Recalibration of the Sunspot-Number: Status Report.
| Title: | Recalibration of the Sunspot-Number: Status Report. |
|---|---|
| Authors: | Clette, F., Lefèvre, L., Chatzistergos, T., Hayakawa, H., Carrasco, V. M. S., Arlt, R., Cliver, E. W., Dudok de Wit, T., Friedli, T. K., Karachik, N., Kopp, G., Lockwood, M., Mathieu, S., Muñoz-Jaramillo, A., Owens, M., Pesnell, D., Pevtsov, A., Svalgaard, L., Usoskin, I. G., van Driel-Gesztelyi, L. |
| Source: | Solar Physics; Mar2023, Vol. 298 Issue 3, p1-59, 59p |
| Abstract: | We report progress on the ongoing recalibration of the Wolf sunspot number ( S N ) and group-sunspot number ( G N ) following the release of version 2.0 of S N in 2015. This report constitutes both an update of the efforts reported in the 2016 Topical Issue of Solar Physics and a summary of work by the International Space Science Institute (ISSI) International Team formed in 2017 to develop optimal S N and G N reconstruction methods while continuing to expand the historical sunspot-number database. Significant progress has been made on the database side while more work is needed to bring the various proposed S N and (primarily) G N reconstruction methods closer to maturity, after which the new reconstructions (or combinations thereof) can be compared with (a) "benchmark" expectations for any normalization scheme (e.g., a general increase in observer normalization factors going back in time), and (b) independent proxy data series such as F10.7 and the daily range of variations of Earth's undisturbed magnetic field. New versions of the underlying databases for S N and G N will shortly become available for years through 2022 and we anticipate the release of the next versions of these two time series in 2024. [ABSTRACT FROM AUTHOR] |
| Subject Terms: | SUN, SPACE sciences, DATABASES, TIME series analysis, SUNSPOTS, MAGNETIC fields |
| Copyright of Solar Physics is the property of Springer Nature and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| ISSN: | 00380938 |
| DOI: | 10.1007/s11207-023-02136-3 |
| Database: | Complementary Index |