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Salakhutdinova, I. I.

doi:10.1023/a:1005265229175

Cited by 12 publications

(5 citation statements)

References 9 publications

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“…It was suggested quite a while ago that the variability of the solar cycle may be a temporal realization of a low-dimensional chaotic system (e.g., Ruzmaikin, 1981). This concept became popular in the early 1990s, when many authors considered solar activity as an example of low-dimensional deterministic chaos, described by the strange attractor (e.g., Kurths and Ruzmaikin, 1990;Ostriakov and Usoskin, 1990;Morfill et al, 1991;Mundt et al, 1991;Rozelot, 1995;Salakhutdinova, 1999;Serre and Nesme-Ribes, 2000;Hanslmeier et al, 2013). Such a process naturally contains randomness, which is an intrinsic feature of the system rather than an independent additive or multiplicative noise.…”

Section: Randomness Vs Regularitymentioning

confidence: 99%

A history of solar activity over millennia

Usoskin

2017

Living Rev Sol Phys

391

241

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Presented here is a review of present knowledge of the long-term behavior of solar activity on a multi-millennial timescale, as reconstructed using the indirect proxy method. The concept of solar activity is discussed along with an overview of the special indices used to quantify different aspects of variable solar activity, with special emphasis upon sunspot number. Over long timescales, quantitative information about past solar activity can only be obtained using a method based upon indirect proxies, such as the cosmogenic isotopes 14 C and 10 Be in natural stratified archives (e.g., tree rings or ice cores). We give an historical overview of the development of the proxy-based method for past solar-activity reconstruction over millennia, as well as a description of the modern state. Special attention is paid to the verification and cross-calibration of reconstructions. It is argued that this method of cosmogenic isotopes makes a solid basis for studies of solar variability in the past on a long timescale (centuries to millennia) during the Holocene. A separate section is devoted to reconstructions of strong solar energetic-particle (SEP) events in the past, that suggest that the present-day average SEP flux is broadly consistent with estimates on longer timescales, and that the occurrence of extra-strong events is unlikely. Finally, the main features of the long-term evolution of solar magnetic activity, including the

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Section: Randomness Vs Regularitymentioning

confidence: 99%

A history of solar activity over millennia

Usoskin

2017

Living Rev Sol Phys

391

241

View full text Add to dashboard Cite

show abstract

Section: Randomness Vs Regularitymentioning

confidence: 99%

A History of Solar Activity over Millennia

Usoskin

2013

Living Rev. Solar Phys.

293

200

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“…This concept became popular in the early 1990s, when many authors considered solar activity as an example of lowdimensional deterministic chaos, described by the strange attractor (e.g., Kurths and Ruzmaikin, 1990;Ostriakov and Usoskin, 1990;Morfill et al, 1991;Mundt et al, 1991;Rozelot, 1995;Salakhutdinova, 1999;Serre and Nesme-Ribes, 2000). Such a process naturally contains randomness, which is an intrinsic feature of the system rather than an independent additive or multiplicative noise.…”

Section: Randomness Vs Regularitymentioning

confidence: 99%

A History of Solar Activity over Millennia

Usoskin

2008

Living Rev. Sol. Phys.

195

200

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Presented here is a review of present knowledge of the long-term behavior of solar activity on a multi-millennial timescale, as reconstructed using the indirect proxy method.The concept of solar activity is discussed along with an overview of the special indices used to quantify different aspects of variable solar activity, with special emphasis upon sunspot number.Over long timescales, quantitative information about past solar activity can only be obtained using a method based upon indirect proxy, such as the cosmogenic isotopes 14 C and 10 Be in natural stratified archives (e.g., tree rings or ice cores). We give an historical overview of the development of the proxy-based method for past solar-activity reconstruction over millennia, as well as a description of the modern state. Special attention is paid to the verification and cross-calibration of reconstructions. It is argued that this method of cosmogenic isotopes makes a solid basis for studies of solar variability in the past on a long timescale (centuries to millennia) during the Holocene.A separate section is devoted to reconstructions of strong solar-energetic-particle (SEP) events in the past, that suggest that the present-day average SEP flux is broadly consistent with estimates on longer timescales, and that the occurrence of extra-strong events is unlikely.Finally, the main features of the long-term evolution of solar magnetic activity, including the statistics of grand minima and maxima occurrence, are summarized and their possible implications, especially for solar/stellar dynamo theory, are discussed.

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Untitled

Cited by 12 publications

References 9 publications

A history of solar activity over millennia

A history of solar activity over millennia

A History of Solar Activity over Millennia

A History of Solar Activity over Millennia

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