Latitude Quenching Nonlinearity in the Solar Dynamo
We compare two candidate nonlinearities for regulating the solar cycle within the Babcock–Leighton paradigm: tilt quenching (whereby the tilt of active regions is reduced in stronger cycles) and latitude quenching (whereby flux emerges at higher latitudes in stronger solar cycles). Digitized histori...
Saved in:
Main Authors: | Anthony R. Yeates, Luca Bertello, Alexander A. Pevtsov, Alexei A. Pevtsov |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad99d0 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
A 22 yr Cycle of the Network Topology of Solar Active Regions
by: Eduardo Flández, et al.
Published: (2025-01-01) -
Correlation of the Flux of Energetic Rays and Particles with the Solar Cycle
by: Ehsan Tavabi, et al.
Published: (2022-10-01) -
Magnetic Flux Emergence and Solar Eruptions in Partially Ionized Plasmas
by: Georgios Chouliaras, et al.
Published: (2025-01-01) -
Detection of a Magnetic Discontinuity in the Upper Solar Chromosphere Associated with a Coronal Loop Brightening Observed by CLASP2.1
by: Donguk Song, et al.
Published: (2025-01-01) -
Experimental dynamos: from models to applications to the geodynamo
by: Pétrélis, François
Published: (2024-12-01)