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pro vyhledávání: '"Timofey Sagitov"'
The number of current sheets observed at 1 AU depends on the corresponding type of the solar wind plasma flow or stream in which current sheets occur. Prior studies have shown that the maximum of the current sheet rate is detected in turbulent and ho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::721f32d3db277294862f4f096b004614
https://doi.org/10.5194/egusphere-egu22-11848
https://doi.org/10.5194/egusphere-egu22-11848
Autor:
Timofey Sagitov
We announce the first open access multi-year database of current sheets systematically identified with the one second cadence at 1 AU. The current sheet list comes from an automated method of current sheet identification that suggests a formalization
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e18c06c1fba334b10a4a0e0f974a0714
https://doi.org/10.5194/egusphere-egu21-8988
https://doi.org/10.5194/egusphere-egu21-8988
Autor:
Timofey Sagitov, Roman Kislov
High speed streams originating from coronal holes are long-lived plasma structures that form corotating interaction regions (CIRs) or stream interface regions (SIRs) in the solar wind. The term CIR is used for streams existing for at least one solar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d22719af72efe1d60b4e01ad1140a3c
https://doi.org/10.5194/egusphere-egu2020-2102
https://doi.org/10.5194/egusphere-egu2020-2102