The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets
Ilya G. UsoskinReSoLVE Centre of Excellence, University of Oulu, 90014, FinlandRainer ArltLeibniz Institute for Astrophysics Potsdam, An der Sternwarte 16, 14482 Potsdam, GermanyEleanna AsvestariReSoLVE Centre of Excellence, University of Oulu, 90014, FinlandEd HawkinsDepartment of Meteorology, University of Reading, UKMaarit KäpyläReSoLVE Centre of Excellence, Department of Computer Science, PO BOX 15400, Aalto University, 00076 Aalto, FinlandGennady A. KovaltsovIoffe Physical-Technical Institute, 194021 St. Petersburg, RussiaNatalie KrivovaMax Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, GermanyMichael LockwoodDepartment of Meteorology, University of Reading, UKKalevi MursulaReSoLVE Centre of Excellence, University of Oulu, 90014, FinlandJezebel O’ReillyMatthew OwensDepartment of Meteorology, University of Reading, UKChris J. ScottDepartment of Meteorology, University of Reading, UKDmitry D. SokoloffIZMIRAN, Moscow, RussiaSami K. SolankiMax Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, GermanyWillie SoonHarvard-Smithsonian Center for Astrophysics, Cambridge, MA, USAJosé M. VaqueroDepartamento de Física, Universidad de Extremadura, Mérida (Badajoz), 10003 Cáceres, Spain
2015en
ABI
Аннотация
Aims. Although the time of the Maunder minimum (1645–1715) is widely known as a period of extremely low solar activity, it is still being debated whether solar activity during that period might have been moderate or even higher than the current solar cycle #24. We have revisited all existing evidence and datasets, both direct and indirect, to assess the level of solar activity during the Maunder minimum.
Перевод пока недоступен
Идентификаторы
Цитирования и источники
Цитирований: 2Использованных источников: 0