Oscillations of the baseline of solar magnetic field and solar irradiance on a millennial timescale
V.V. Zharkova, S.J. Shepherd, E. Popova

TL;DR
This paper investigates millennial-scale oscillations in the solar magnetic field and irradiance, revealing long-term cycles and their potential impact on Earth's climate, including a possible future increase in global temperature.
Contribution
It introduces a 100,000-year double dynamo model and identifies a 1950-year super-grand cycle linked to solar inertial motion, advancing understanding of solar-terrestrial interactions.
Findings
Confirmed strong oscillations in solar activity at 11-year and 350-400-year cycles.
Discovered a 1950-year super-grand cycle in baseline magnetic field oscillations.
Linked baseline magnetic field oscillations to potential terrestrial temperature increases.
Abstract
Recently discovered long-term oscillations of the solar background magnetic field associated with double dynamo waves generated in inner and outer layers of the Sun indicate that the solar activity is heading in the next three decades (2019-2055) to a Modern grand minimum similar to Maunder one. On the other hand, a reconstruction of solar total irradiance suggests that since the Maunder minimum there is an increase in the cycle-averaged total solar irradiance (TSI) by a value of about closely correlated with an increase of the baseline (average) terrestrial temperature. In order to understand these two opposite trends, we calculated the double dynamo summary curve of magnetic field variations backward one hundred thousand years allowing us to confirm strong oscillations of solar activity in regular (11 year) and recently reported grand (350-400 year) solar cycles…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Geomagnetism and Paleomagnetism Studies
