Morphology and dynamics of photospheric and chromospheric magnetic fields

Details Morphology and dynamics of photospheric and chromospheric magnetic fields Morphology and dynamics of photospheric and chromospheric magnetic fields

2009-12-17

arxiv.org/abs/0912.3285v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

to appear in "The Second Hinode Science Meeting: Beyond Discovery - Toward Understanding", ASP Conference Series, Vol. 415, ed

Scientific paper

We use joint observations obtained with the Hinode space observatory and the Interferometric Bidimensional Spectrometer (IBIS) installed at the DST of the NSO/SP to investigate the morphology and dynamics of (a) non-magnetic and (b) magnetic regions in the fluctosphere. In inter-network regions with no significant magnetic flux contributions above the detection limit of IBIS, we find intensity structures with similar characteristics as those seen in numerical simulations by Wedemeyer-B\"ohm (2008). The magnetic flux elements in the network are stable and seem to resemble the spatially extended counterparts to the underlying photospheric magnetic elements. We will explain some of the difficulties in deriving the magnetic field vector from observations of the fluctosphere.

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