activity
20092022
most citedNew dynamo pattern revealed by solar helical magnetic fields

86 citations · 212 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2022★ 11 cited

Solar wind modeling with the Alfven Wave Solar atmosphere Model driven by HMI-based Near-Real-Time maps by the National Solar Observatory

Nishtha Sachdeva, Ward B Manchester, Igor Sokolov +6

We explore model performance for the Alfven Wave Solar atmosphere Model (AWSoM) with near-real-time (NRT) synoptic maps of the photospheric vector magnetic field. These maps, produ…

astro-ph.SR2018★ 29 cited

The magnetic field vector of the Sun-as-a-star. II. Evolution of the large-scale vector field through activity cycle 24

A. A. Vidotto, L. Lehmann, M. Jardine +1

In the present work, we investigate how the large-scale magnetic field of the Sun, in its three vector components, has evolved during most of cycle 24, from 2010 Jan to 2018 Apr. T…

astro-ph.SR2016

Solar Physics Research in the Russian Subcontinent - Current Status and Future

A. A. Pevtsov, Yu. A. Nagovitsyn, A. G. Tlatov +1

Modern research in solar physics in Russia is a multifaceted endeavor, which includes multi-wavelength observations from the ground- and space-based instruments, extensive theoreti…

astro-ph.SR2016

The reversal of the Sun's magnetic field in cycle 24

Alexander V. Mordvinov, Alexei A. Pevtsov, Luca Bertello +1

Analysis of synoptic data from the Vector Stokes Magnetograph (VSM) of the Synoptic Optical Long-term Investigations of the Sun (SOLIS) and the NASA/NSO Spectromagnetograph (SPM) a…

astro-ph.SR2014★ 19 cited

Magnetic helicity of global field in cycles 23 and 24

V. V. Pipin, A. A. Pevtsov

For the first time we reconstruct the magnetic helicity density of global axisymmetric field of the Sun using method proposed by Brandenburg et al. (2003) and Pipin et al. (2013).…

astro-ph.SR2013★ 45 cited

Uncertainties in Solar Synoptic Magnetic Flux Maps

L. Bertello, A. A. Pevtsov, G. J. D. Petrie +1

Magnetic flux synoptic charts are critical for reliable modeling of the corona and heliosphere. Until now, however, these charts were provided without any estimate of uncertainties…