papers

Publications (13)

astro-ph.SR2016

Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333)

Ian Waite, Stephen Marsden, Brad Carter +6

The magnetic fields, activity and dynamos of young solar-type stars can be empirically studied using time-series of spectropolarimetric observations and tomographic imaging techniq…

astro-ph.SR2016

The BRITE spectropolarimetric program

Coralie Neiner, Gregg Wade, Stephen Marsden +1

A high-resolution spectropolarimetric survey of all (573) stars brighter than magnitude V=4 has been undertaken with Narval at TBL, ESPaDOnS at CFHT, and HarpsPol at ESO, as a grou…

astro-ph.SR2011

High Resolution Spectroscopy and Spectropolarimetry of some late F-/early G-type sun-like stars as targets for Zeeman Doppler imaging

Ian Waite, Stephen Marsden, Brad Carter +4

High resolution spectroscopy and spectropolarimetry have been undertaken at the Anglo-Australian Telescope in order to identify suitable targets for magnetic studies of young sun-l…

astro-ph.SR2026

Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. III. Comparison between Starspot Mapping, Zeeman Doppler Imaging, and Multiwavelength Variability

Kai Ikuta, Kosuke Namekata, Pascal Petit +12

Recent simultaneous multiwavelength observations of a nearby young solar-type star EK Dra in the optical, H spectrum, and X-ray, have provided evidence for stellar prominence e…

astro-ph.SR2024

Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-Driven Modeling and Observed Magnetic Environment

Kosuke Namekata, Kai Ikuta, Pascal Petit +15

EK Draconis, a nearby young solar-type star (G1.5V, 50-120 Myr), is known as one of the best proxies for inferring the environmental conditions of the young Sun. The star frequentl…

astro-ph.SR2015

Magnetic fields on young, moderately rotating Sun-like stars - I: HD~35296 and HD~29615

Ian Waite, Stephen Marsden, Bradley Carter +4

Observations of the magnetic fields of young solar-type stars provide a way to investigate the signatures of their magnetic activity and dynamos. Spectropolarimetry enables the stu…

astro-ph.SR2013

Starspots on Young Solar-Type Stars

Carolyn Brown, Brad Carter, Stephen Marsden +1

Doppler Imaging of starspots on young solar analogues is a way to investigate the early history of solar magnetic activity by proxy. Doppler images of young G-dwarfs have yielded t…

astro-ph.SR2021

Coronal mass ejections and type II radio emission variability during a magnetic cycle on the solar-type star Eridani

Dúalta Ó Fionnagáin, Robert D. Kavanagh, Aline A. Vidotto +5

We simulate possible stellar coronal mass ejection (CME) scenarios over the magnetic cycle of Eridani (18 Eridani; HD 22049). We use three separate epochs from 2008, 2011, and…

astro-ph.SR2023

Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares

Kosuke Namekata, Vladimir S. Airapetian, Pascal Petit +14

Young solar-type stars frequently produce superflares, serving as a unique window into the young Sun-Earth environments. Large solar flares are closely linked to coronal mass eject…

astro-ph.IM2019

Minerva-Australis I: Design, Commissioning, & First Photometric Results

Brett Addison, Duncan J. Wright, Robert A. Wittenmyer +35

The Minerva-Australis telescope array is a facility dedicated to the follow-up, confirmation, characterisation, and mass measurement of bright transiting planets discovered by the…

astro-ph.SR2010

Young Stars in the Time Domain: A Cool Stars 16 Splinter Summary

Kevin R. Covey, Peter Plavchan, Fabienne Bastien +6

Variability is a defining characteristic of young stellar systems, and optical variability has been heavily studied to select and characterize the photospheric properties of young…

physics.plasm-ph2024

Multi-objective Bayesian optimization for design of Pareto-optimal current drive profiles in STEP

Theodore Brown, Stephen Marsden, Vignesh Gopakumar +3

The safety factor profile is a key property in determining the stability of tokamak plasmas. To design the safety factor profile in the United Kingdom's proposed Spherical Tokamak…

astro-ph.SR2013

A Bcool spectropolarimetric survey of over 150 solar-type stars

Stephen Marsden, Pascal Petit, Sandra Jeffers +3

As part of the Bcool project, over 150 solar-type stars chosen mainly from planet search databases have been observed between 2006 and 2013 using the NARVAL and ESPaDOnS spectropol…