Revisited sunspot data: A new scenario for the onset of the Maunder minimum
arXiv:1103.1520 · doi:10.1088/2041-8205/731/2/L24
Abstract
Maunder Minimum forms an archetype for the Grand minima, and detailed knowledge of its temporal development has important consequences for the solar dynamo theory dealing with long-term solar activity evolution. Here we reconsider the current paradigm of the Grand minimum general scenario by using newly recovered sunspot observations by G. Marcgraf and revising some earlier uncertain data for the period 1636--1642, i.e., one solar cycle before the beginning of the Maunder Minimum. The new and revised data dramatically change the magnitude of the sunspot cycle just before the Maunder Minimum, from 60--70 down to about 20, implying a possibly gradual onset of the Minimum with reduced activity started two cycles before it. This revised scenario of the Maunder Minimum changes, through the paradigm for Grand solar/stellar activity minima, the observational constraint on the solar/stellar dynamo theories focused on long-term studies and occurrence of Grand minima.
8 pages, 2 figures, accepted for publication in ApJ Letters
References in corpus (3)
Cited by in corpus (42)
- The Solar Cycle
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- The Maunder minimum (1645--1715) was indeed a Grand minimum: A reassessment of multiple datasets
- A Revised Collection of Sunspot Group Numbers
- A New Calibrated Sunspot Group Series Since 1749: Statistics of Active Day Fractions
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- Re-calibration of the Sunspot Number: Status Report
- Level and length of cyclic solar activity during the Maunder minimum as deduced from the active day statistics
- Models for the long-term variations of solar activity
- A Stochastically Forced Time Delay Solar Dynamo Model: Self-Consistent Recovery from a Maunder-like Grand Minimum Necessitates a Mean-Field Alpha Effect
- Variations of the solar cycle profile in a solar dynamo with fluctuating dynamo governing parameters
- Studies of grand minima in sunspot cycles from a flux transport solar dynamo model
- An Assessment of Sunspot Number Data Composites over 1845-2014
- Thaddäus Derfflinger's sunspot observations during 1802-1824: A primary reference to understand the Dalton Minimum
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- Sunspots during the Maunder Minimum from Machina Coelestis by Hevelius
- Sunspot latitudes during the Maunder Minimum: a machine-readable catalogue from previous studies
- A Simple Method to Check the Reliability of Annual Sunspot Number in the Historical Period 1610-1847
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- Revised Group Sunspot Number for 1640, 1652, and 1741
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- The umbra-penumbra area ratio of sunspots during the Maunder Minimum
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- Revisiting Christoph Scheiner's Sunspot Records: a New Perspective on Solar Activity of the Early Telescopic Era
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- Solar Angular Momentum Loss Over the Past Several Millennia
- The Sunspot Catalogues of Carrington, Peters, and de la Rue: Quality Control and Machine-readable Versions
- Daniel Mögling's sunspot observations in 1626 - 1629: A manuscript reference for the solar activity before the Maunder Minimum
- Sunspot Observations by Hisako Koyama: 1945-1996
- Revisiting Kunitomo's Sunspot Drawings during 1835-1836 in Japan
- Sunspot observations by Charles Malapert during the period 1618-1626: a key dataset to understand solar activity before the Maunder minimum
- Newly found sunspot observations by Peter Becker from Rostock for 1708, 1709, and 1710
- Could a Hexagonal Sunspot Have Been Observed During the Maunder Minimum?
- Dynamo models of grand minima
- An analysis of the solar differential rotation in solar cycle No. 19 (1954-1964) determined using Kanzelhoehe sunspot group positions