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In the solar photosphere, many properties of coronal holes (CHs) are notknown, especially vector magnetic fields. Using observations from Hinode, we investigate vector magnetic fields, current densiti...
Coronal holes and interplanetary disturbances are important aspects of the physics of the Sun and heliosphere. Interplanetary disturbances are identified as an increase in the density turbulence compa...
Recently, we suggested that the source of ion heating in solar coronal holes is small-scale reconnection events (microflares) at the coronal base. The microflares launch intermittent heat flux up into...
We investigate the effect of viscosity and magnetic diffusivity on the oblique propagation and dissipation of Alfv´en waves with respect to the normal outward direction, making use of MHD equa...
Coronal holes and interplanetary disturbances are important aspects of the physics of the Sun and heliosphere. Interplanetary disturbances are identified as an increase in the density turbulence comp...
We investigate the effect of viscosity and magnetic diffusivity on the oblique propagation and dissipation of Alfv´en waves with respect to the normal outward direction, making use of MHD equati...

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