activity
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 2020Show all

5 papers · 1 filter

astro-ph.SR2020★ 13 cited

The Contribution of Alpha Particles to the Solar Wind Angular Momentum Flux in the Inner Heliosphere

Adam J. Finley, Michael D. McManus, Sean P. Matt +14

An accurate assessment of the Sun's angular momentum (AM) loss rate is an independent constraint for models that describe the rotation evolution of Sun-like stars. In-situ measurem…

astro-ph.SR2020★ 16 cited

The Solar Wind Angular Momentum Flux as Observed by Parker Solar Probe

Adam J. Finley, Sean P. Matt, Victor Réville +9

The long-term evolution of the Sun's rotation period cannot be directly observed, and is instead inferred from trends in the measured rotation periods of other Sun-like stars. Assu…

astro-ph.SR2020★ 12 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.SR2020★ 40 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★ 12 cited

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…