activity
20172020
most citedEstimating magnetic filling factors from Zeeman-Doppler magnetograms

93 citations · 295 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.SR202012 cited

Parker Solar Probe Observations of Suprathermal Electron Flux Enhancements Originating from Coronal Hole Boundaries

Allan R Macneil, Mathew J Owens, Laura Berčič +1

Reconnection between pairs of solar magnetic flux elements, one open and the other a closed loop, is theorised to be a crucial process for both maintaining the structure of the cor…

astro-ph.SR202040 cited

Alfvén-wave driven magnetic rotator winds from low-mass stars I: rotation dependences of magnetic braking and mass-loss rate

Munehito Shoda, Takeru K. Suzuki, Sean P. Matt +7

Observations of stellar rotation show that low-mass stars lose angular momentum during the main sequence. We simulate the winds of Sun-like stars with a range of rotation rates, co…

astro-ph.SR2020

How much do underestimated field strengths from Zeeman-Doppler imaging affect spin-down torque estimates?

Victor See, Lisa Lehmann, Sean P. Matt +1

Numerous attempts to estimate the rate at which low-mass stars lose angular momentum over their lifetimes exist in the literature. One approach is to use magnetic maps derived from…

astro-ph.SR201927 cited

Direct Detection of Solar Angular Momentum Loss with the Wind Spacecraft

Adam J. Finley, Amy L. Hewitt, Sean P. Matt +3

The rate at which the solar wind extracts angular momentum from the Sun has been predicted by theoretical models for many decades, and yet we lack a conclusive measurement from in-…

astro-ph.SR201957 cited

Do non-dipolar magnetic fields contribute to spin-down torques?

Victor See, Sean P. Matt, Adam J. Finley +14

Main sequence low-mass stars are known to spin-down as a consequence of their magnetised stellar winds. However, estimating the precise rate of this spin-down is an open problem. T…

astro-ph.SR2019

Solar Angular Momentum Loss Over the Past Several Millennia

Adam J. Finley, Siddhant Deshmukh, Sean P. Matt +2

The Sun and Sun-like stars lose angular momentum to their magnetised stellar winds. This braking torque is coupled to the stellar magnetic field, such that changes in the strength…