Redefining the limit dates for the Maunder Minimum
J. M. Vaquero, R. M. Trigo

TL;DR
This paper refines the chronological boundaries of the Maunder Minimum, a period of low solar activity, using new proxy data to distinguish between the core and extended phases of this solar phenomenon.
Contribution
It introduces a new, more precise timeline for the Maunder Minimum, differentiating the core from the extended period based on recent proxy analyses.
Findings
Core 'Deep Maunder Minimum' from 1645 to 1700
Extended Maunder Minimum from 1618 to 1723
Transition periods identified within the extended timeline
Abstract
The Maunder Minimum corresponds to a prolonged minimum of solar activity a phenomenon that is of particular interest to many branches of natural and social sciences commonly considered to extend from 1645 until 1715. However, our knowledge of past solar activity has improved significantly in recent years and, thus, more precise dates for the onset and termination of this particularly episode of our Sun can be established. Based on the simultaneous analysis of distinct proxies we propose a redefinition of the Maunder Minimum period with the core "Deep Maunder Minimum" spanning from 1645 to 1700 (that corresponds to the Grand Minimum state) and a wider "Extended Maunder Minimum" for the longer period 1618-1723 that includes the transition periods.
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