Near-Earth heliospheric magnetic field intensity since 1750: 1. Sunspot and geomagnetic reconstructions

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Global solar wind variations over the last four centuries.Space climate and space weather over the past 400 years: 1. The power input to the magnetosphere Near-Earth heliospheric magnetic field intensity since 1750: 2. Cosmogenic radionuclide reconstructions

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Near-Earth heliospheric magnetic field intensity since 1750: 1. Sunspot and geomagnetic reconstructions

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wetenschappelijk artikel

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наукова стаття, опублікована в липні 2016

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Near-Earth heliospheric magnet ...... nd geomagnetic reconstructions

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Near-Earth heliospheric magnet ...... nd geomagnetic reconstructions

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Near-Earth heliospheric magnet ...... nd geomagnetic reconstructions

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Near-Earth heliospheric magnet ...... nd geomagnetic reconstructions

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Near-Earth heliospheric magnet ...... nd geomagnetic reconstructions

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Near-Earth heliospheric magnet ...... nd geomagnetic reconstructions

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Near-Earth heliospheric magnet ...... nd geomagnetic reconstructions

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P2093

A. Rouillard

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D. Passos

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E. Cliver

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I. Usoskin

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J. Beer

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K. G. McCracken

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M. J. Owens

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P. Riley

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Y-M. Wang

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P2860

Solar Influence on Global and Regional Climates

Modeling the Sun’s Magnetic Field and Irradiance since 1713

Regional climate impacts of a possible future grand solar minimum.

The maunder minimum.

Solar Plasma Experiment.

Evolution of the solar irradiance during the Holocene

The Heliospheric Magnetic Field

A doubling of the Sun's coronal magnetic field during the past 100 years

Reconstruction and Prediction of Variations in the Open Solar Magnetic Flux and Interplanetary Conditions

The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets

P304

6048-6063

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P31

scholarly article

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10.1002/2016JA022529

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http://www.w3.org/2001/XMLSchema#string

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121

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Mike Lockwood

Luke Barnard

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2016-07-01T00:00:00Z

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Near-Earth heliospheric magnetic field intensity since 1750: 1. Sunspot and geomagnetic reconstructions

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P2860

P2860

Near-Earth heliospheric magnetic field intensity since 1750: 1. Sunspot and geomagnetic reconstructions

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P2093

P2860

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P433

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P2093

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P433

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