Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/8269
Title: | Long-term Evolution of Magnetic Field Proxies as Deduced from Archival Data |
Authors: | Banerjee, D Bibhuti Kumar Jha Mandal, Sudip Chatterjee, Subhamoy Hegde, M KoSO Digitization Team |
Keywords: | Sun: magnetic fields Sun: photosphere Sun: chromosphere Catalogs |
Issue Date: | 2023 |
Publisher: | Cambridge University Press on behalf of International Astronomical Union |
Citation: | Proceedings of the International Astronomical Union, Vol. 18, No. 372, pp. 84-85 |
Abstract: | Regular observations of the solar magnetic field are available only for about the last five cycles. Thus, to understand the origin of the variation of the solar magnetic field, it is essential to reconstruct the magnetic field for the past cycles, utilizing the proxies of the magnetic field from other data sets. Long-term uniform observations for the past 100 yrs, as recorded at the Kodaikanal Solar Observatory (KoSO), in multi-wavelengths provide such an opportunity. Various automatic techniques have been developed to extract these features from KoSO data. We analyzed the properties of these extracted features to understand global solar magnetism in the past. |
Description: | Restricted Access |
URI: | http://hdl.handle.net/2248/8269 |
ISSN: | 1743-9221 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Long-term Evolution of Magnetic Field Proxies as Deduced from Archival Data.pdf Restricted Access | 673.56 kB | Adobe PDF | View/Open Request a copy |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.