activity
20072025
most citedOn Predicting the Solar Cycle using Mean-Field Models

100 citations · 539 across the 30 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2020★ 1 cited

On the saturation mechanism of the fluctuation dynamo at

Amit Seta, Paul J. Bushby, Anvar Shukurov +1

The presence of magnetic fields in many astrophysical objects is due to dynamo action, whereby a part of the kinetic energy is converted into magnetic energy. A turbulent dynamo th…

astro-ph.GA2019★ 15 cited

The supernova-regulated ISM -- VI. Magnetic effects on the structure of the interstellar medium

C. C. Evirgen, F. A. Gent, A. Shukurov +2

We explore the effect of magnetic fields on the vertical distribution and multiphase structure of the supernova-driven interstellar medium (ISM) in simulations that admit dynamo ac…

astro-ph.GA2018

On energy equipartition between cosmic rays and magnetic fields

Amit Seta, Anvar Shukurov, Paul J. Bushby +1

Interpretations of synchrotron observations often assume a tight correlation between magnetic and cosmic ray energy densities. We examine this assumption using both test-particle s…

astro-ph.GA2018★ 39 cited

A physical approach to modelling large-scale galactic magnetic fields

Anvar Shukurov, Luiz Felippe S. Rodrigues, Paul J. Bushby +2

A convenient representation of the structure of the large-scale galactic magnetic field is required for the interpretation of polarization data in the sub-mm and radio ranges, in b…

astro-ph.GA2017★ 46 cited

Relative distribution of cosmic rays and magnetic fields

Amit Seta, Anvar Shukurov, Toby S. Wood +2

Synchrotron radiation from cosmic rays is a key observational probe of the galactic magnetic field. Interpreting synchrotron emission data requires knowledge of the cosmic ray numb…

astro-ph.GA2017★ 18 cited

Topological signatures of interstellar magnetic fields - I. Betti numbers and persistence diagrams

Irina Makarenko, Anvar Shukurov, Robin Henderson +3

The interstellar medium (ISM) is a magnetised system in which transonic or supersonic turbulence is driven by supernova explosions. This leads to the production of intermittent, fi…