631 citations · 2.3k across the 40 of their papers we have counts for
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The energy budget of stellar magnetic fields: comparing non-potential simulations and observations
L. T. Lehmann, M. M. Jardine, A. A. Vidotto +8
The magnetic geometry of the surface magnetic fields of more than 55 cool stars have now been mapped using spectropolarimetry. In order to better understand these observations, we…
Origin and Ion Charge State Evolution of Solar Wind Transients during 4 -- 7 August 2011
D. Rodkin, F. Goryaev, P. Pagano +5
We present study of the complex event consisting of several solar wind transients detected by Advanced Composition Explorer (ACE) on 4 -- 7 August 2011, that caused a geomagnetic s…
Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves
D. B. Jess, V. E. Reznikova, R. S. I. Ryans +9
Sunspots on the surface of the Sun are the observational signatures of intense manifestations of tightly packed magnetic field lines, with near-vertical field strengths exceeding 6…
Magnetic reconnection between a solar filament and nearby coronal loops
Leping Li, Jun Zhang, Hardi Peter +5
Magnetic reconnection, the rearrangement of magnetic field topology, is a fundamental physical process in magnetized plasma systems all over the universe1,2. Its process is difficu…
Stellar Coronal Response to Differential Rotation and Flux Emergence
G. P. S. Gibb, D. H. Mackay, M. M. Jardine +1
We perform a numerical parameter study to determine what effect varying differential rotation and flux emergence has on a star's non-potential coronal magnetic field. In particular…