Dynamo models of the solar cycle

P Charbonneau - Living Reviews in Solar Physics, 2020 - Springer
This paper reviews recent advances and current debates in modeling the solar cycle as a
hydromagnetic dynamo process. Emphasis is placed on (relatively) simple dynamo models …

Solar cycle observations

A Norton, R Howe, L Upton, I Usoskin - Space Science Reviews, 2023 - Springer
We describe the defining observations of the solar cycle that provide constraints for the
dynamo processes operating within the Sun. Specifically, we report on the following topics …

[HTML][HTML] The solar orbiter mission-science overview

D Müller, OCS Cyr, I Zouganelis, HR Gilbert… - Astronomy & …, 2020 - aanda.org
Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …

The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes

Y Bekki, RH Cameron, L Gizon - Science Advances, 2024 - science.org
Rapidly rotating fluids have a rotation profile that depends only on the distance from the
rotation axis, in accordance with the Taylor-Proudman theorem. Although the Sun was …

Analysis of solar hemispheric chromosphere properties using the kodaikanal observatory Ca–K index

P Chowdhury, R Belur, L Bertello… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Kodaikanal Observatory has provided long-term synoptic observations of
chromospheric activities in the Ca ii K line (393.34 nm) since 1907. This article investigates …

Tidally forced planetary waves in the tachocline of solar-like stars

GM Horstmann, G Mamatsashvili… - The Astrophysical …, 2023 - iopscience.iop.org
Can atmospheric waves in planet-hosting solar-like stars substantially resonate to tidal
forcing, perhaps at a level of impacting the space weather or even being dynamo-relevant …

Space weather challenge and forecasting implications of Rossby waves

M Dikpati, SW McIntosh - Space Weather, 2020 - Wiley Online Library
Rossby waves arise in thin layers within fluid regions of stars and planets. These global
wave‐like patterns occur due to the variation in Coriolis forces with latitude. In the past …

Rieger, Schwabe, Suess-de Vries: the sunny beats of resonance

F Stefani, GM Horstmann, M Klevs, G Mamatsashvili… - Solar Physics, 2024 - Springer
We propose a self-consistent explanation of Rieger-type periodicities, the Schwabe cycle,
and the Suess-de Vries cycle of the solar dynamo in terms of resonances of various wave …

On the connection between Rieger-type and magneto-Rossby waves driving the frequency of the large solar eruptions during solar cycles 19–25

MB Korsós, M Dikpati, R Erdélyi, J Liu… - The Astrophysical …, 2023 - iopscience.iop.org
Global solar activity variation mainly occurs over about an 11 yr cycle. However, both longer
and shorter periodicities than the solar cycle are also present in many different solar activity …

Rossby waves in astrophysics

TV Zaqarashvili, M Albekioni, JL Ballester, Y Bekki… - Space Science …, 2021 - Springer
Rossby waves are a pervasive feature of the large-scale motions of the Earth's atmosphere
and oceans. These waves (also known as planetary waves and r-modes) also play an …