Millenium-scale sunspot number reconstruction: Evidence for an unusually active 
Sun since the 1940s

Usoskin, I.; Solanki, S. K.; Schüssler, M.; Mursula, K.; Alanko, K.

doi:10.1103/PhysRevLett.91.211101

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Millenium-scale sunspot number reconstruction: Evidence for an unusually active Sun since the 1940s

Usoskin, I., Solanki, S. K., Schüssler, M., Mursula, K., & Alanko, K. (2003). Millenium-scale sunspot number reconstruction: Evidence for an unusually active Sun since the 1940s. Physical Review Letters, 91: 211101. doi:10.1103/PhysRevLett.91.211101.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-EE85-4 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-EE86-2

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Usoskin, I., Author
Solanki, S. K.^{1, 2}, Author
Schüssler, M.^{1, 2}, Author
Mursula, K., Author
Alanko, K., Author

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1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291

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MPIS_GROUPS: Sun and Heliosphere

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Dates: Date issued: 2003

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Rev. Type: Peer

Identifiers: DOI: 10.1103/PhysRevLett.91.211101
BibTex Citekey: Usoskin:2003-118

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Title: Physical Review Letters

Source Genre: Journal

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Pages: - Volume / Issue: 91 Sequence Number: 211101 Start / End Page: - Identifier: -