activity
20002017
most citedThe Role of Magnetic Helicity Transport in Nonlinear Galactic Dynamos

82 citations · 756 across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2017★ 8 cited

Parity fluctuations in stellar dynamos

D. L. Moss, D. D. Sokoloff

Observations of the solar butterfly diagram from sunspot records suggest persistent fluctuation in parity, away from the overall, approximately dipolar structure. We use a simple m…

astro-ph.GA2016★ 9 cited

Galactic winds and the origin of large-scale magnetic fields

David Moss, Dmitri Sokoloff

Observations of dwarf galaxies suggest the presence of large-scale magnetic fields. However the size and slow rotation of these galaxies appear insufficient to support a mean-field…

astro-ph.HE2016★ 29 cited

Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems

David Moss, Dmitri Sokoloff, Valery Suleimanov

Magnetic fields are important for accretion disc structure. Magnetic fields in a disc system may be transported with the accreted matter. They can be associated with either the cen…

astro-ph.GA2015★ 21 cited

The formation of regular interarm magnetic fields in spiral galaxies

David Moss, Rodion Stepanov, Marita Krause +2

Observations of regular magnetic fields in several nearby galaxies reveal magnetic arms situated between the material arms. The nature of these magnetic arms is a topic of active d…

astro-ph.SR2015★ 25 cited

Towards understanding dynamo action in M dwarfs

D. Shulyak, D. Sokoloff, L. Kitchatinov +1

Recent progress in observational studies of magnetic activity in M dwarfs urgently requires support from ideas of stellar dynamo theory. We propose a strategy to connect observatio…

astro-ph.GA2014★ 13 cited

Magnetic fields near the peripheries of galactic discs

E. Mikhailov, A. Kasparova, D. Moss +3

Magnetic fields are observed beyond the peripheries of optically detected galactic discs, while numerical models of their origin and the typical magnitudes are still absent. Previo…