Space climate and space weather over the past 400 years: 2. Proxy indicators of geomagnetic storm and substorm
arXiv:1801.02434 · doi:10.1051/swsc/2017048
Abstract
Using the reconstruction of power input to the magnetosphere given in Paper 1 (arXiv:1708.04904), we reconstruct annual means of geomagnetic indices over the past 400 years to within a 1-sigma error of +/-20 pc. In addition, we study the behaviour of the lognormal distribution of daily and hourly values about these annual means and show that we can also reconstruct the fraction of geomagnetically-active (storm-like) days and (substorm-like) hours in each year to accuracies of 50-60 pc. The results are the first physics-based quantification of the space weather conditions in both the Dalton and Maunder minima. We predict terrestrial disturbance levels in future repeats of these minima, allowing for the weakening of Earth's dipole moment.
References in corpus (7)
- The Maunder minimum (1645--1715) was indeed a Grand minimum: A reassessment of multiple datasets
- Evolution of the solar magnetic flux on time scales of years to millenia
- An Assessment of Sunspot Number Data Composites over 1845-2014
- A new method to estimate annual solar wind parameters and contributions of different solar wind structures to geomagnetic activity
- Tests of Sunspot Number Sequences: 2. Using Geomagnetic and Auroral Data
- The lost sunspot cycle: New support from Be10 measurements
- Probability density functions for the variable solar wind near the solar cycle minimum
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