Could a change in magnetic field geometry cause the break in the wind-activity relation?
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The evolution of surface magnetic fields in young solar-type stars II: the early main sequence (250–650 Myr)★Studying stellar spin-down with Zeeman–Doppler magnetogramsThe energy budget of stellar magnetic fields: comparing non-potential simulations and observationsThe connection between stellar activity cycles and magnetic field topologyMagnetism, dynamo action and the solar-stellar connectionAn improved age–activity relationship for cool stars older than a gigayear
P2860
Could a change in magnetic field geometry cause the break in the wind-activity relation?
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wetenschappelijk artikel
@nl
наукова стаття, опублікована в жовтні 2015
@uk
name
Could a change in magnetic field geometry cause the break in the wind-activity relation?
@en
Could a change in magnetic field geometry cause the break in the wind-activity relation?
@nl
type
label
Could a change in magnetic field geometry cause the break in the wind-activity relation?
@en
Could a change in magnetic field geometry cause the break in the wind-activity relation?
@nl
prefLabel
Could a change in magnetic field geometry cause the break in the wind-activity relation?
@en
Could a change in magnetic field geometry cause the break in the wind-activity relation?
@nl
P2093
P2860
P356
P1476
Could a change in magnetic field geometry cause the break in the wind-activity relation?
@en
P2093
A. A. Vidotto
E. Hébrard
J.-F. Donati
M. Jardine
S. Boro Saikia
S. C. Marsden
S. V. Jeffers
P2860
P304
P356
10.1093/MNRASL/SLV147
P577
2015-10-29T00:00:00Z
P818
1509.08751
P819
2016MNRAS.455L..52V