activity
19982023
most citedThe Maunder minimum (1645--1715) was indeed a Grand minimum: A reassessment of multiple datasets

208 citations · 2.1k across the 47 of their papers we have counts for

collaborators

47 papers

astro-ph.SR2023★ 51 cited

Evolution of solar and stellar dynamo theory

Paul Charbonneau, Dmitry Sokoloff

In this paper, written as a general historical and technical introduction to the various review papers collected in the special issue ``Solar and Stellar Dynamo: A New Era'', we re…

astro-ph.SR2022★ 6 cited

Migrating Dynamo Waves and Consequences for Stellar Current Sheets

E. Maiewski, H. Malova, V. Popov +2

We study the relation between stellar dynamo-wave propagation and the structure of the stellar magnetic field. Modeling dynamo waves by the well-known Parker migratory dynamo, we v…

astro-ph.SR2021★ 32 cited

Solar large-scale magnetic field and cycle patterns in solar dynamo

V. N. Obridko, V. V. Pipin, D. D. Sokoloff +1

We compare spectra of the zonal harmonics of the large-scale magnetic field of the Sun using observation results and solar dynamo models. The main solar activity cycle as recorded…

astro-ph.SR2020★ 17 cited

A Catalog of Bipolar Active Regions Violating the Hale Polarity Law, 1989-2018

A. Zhukova, A. Khlystova, V. Abramenko +1

There is no list of bipolar active regions (ARs) with reverse polarity (anti-Hale regions), although statistical investigations of such ARs (bearing the imprint of deep subphotosph…

astro-ph.SR2020★ 15 cited

Shape of solar cycles and mid-term solar activity oscillations

D. D. Sokoloff, A. S. Shibalova, V. N. Obridko +1

The evolution of the solar activity comprises, apart from the well-known 11-year cycle, various temporal scales ranging from months up to the secondary cycles known as mid-term osc…

astro-ph.SR2020★ 2 cited

Estimates of current helicity and tilt of solar active regions and Joy's law

K. Kuzanyan, N. Kleeorin, I. Rogachevskii +2

The tilt angle, current helicity and twist of solar magnetic fields can be observed in solar active regions. We carried out estimates of these parameters by two ways. Firstly, we c…