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20172026
most citedEstimating magnetic filling factors from Zeeman-Doppler magnetograms

93 citations · 731 across the 35 of their papers we have counts for

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Showing 2019Show all

5 papers · 1 filter

astro-ph.SR2019★ 27 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.SR2019★ 57 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★ 20 cited

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…

astro-ph.SR2019★ 18 cited

The Effect of Magnetic Variability on Stellar Angular Momentum Loss II: The Sun, 61 Cygni A, Eridani, Bootis A and Bootis A

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

The magnetic fields of low-mass stars are observed to be variable on decadal timescales, ranging in behaviour from cyclic to stochastic. The changing strength and geometry of the m…

astro-ph.SR2019★ 93 cited

Estimating magnetic filling factors from Zeeman-Doppler magnetograms

Victor See, Sean P. Matt, Colin P. Folsom +15

Low-mass stars are known to have magnetic fields that are believed to be of dynamo origin. Two complementary techniques are principally used to characterise them. Zeeman-Doppler im…