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Magneto-static modeling from Sunrise/IMaX: Application to an active region observed with Sunrise II

Listed in National Center for Atmospheric Research

Magneto-static models may overcome some of the issues facing force-free magnetic field extrapolations.

Description

So far they have seen limited use and have faced problems when applied to quiet-Sun data. Here we present a first application to an active region.

We use solar vector magnetic field measurements gathered by the IMaX polarimeter during the flight of the SUNRISE balloon-borne solar observatory in 2013 June as boundary conditions for a magneto-static model of the higher solar atmosphere above an active region. The IMaX data are embedded in active region vector magnetograms observed with SDO/HMI. This work continues our magneto-static extrapolation approach, which was applied earlier to a quiet-Sun region observed with SUNRISE I. In an active region the signal-to-noise-ratio in the measured Stokes parameters is considerably higher than in the quiet-Sun and consequently the IMaX measurements of the horizontal photospheric magnetic field allow us to specify the free parameters of the model in a special class of linear magneto-static equilibria.

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The high spatial resolution of IMaX (110-130 km, pixel size 40 km) enables us to model the non-force-free layer between the photosphere and the mid-chromosphere vertically by about 50 grid points. In our approach we can incorporate some aspects of the mixed beta layer of photosphere and chromosphere, e.g., taking a finite Lorentz force into account, which was not possible with lower-resolution photospheric measurements in the past.

The linear model does not, however, permit us to model intrinsic nonlinear structures like strongly localized electric currents.

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National Center for Atmospheric Research982b4199-b08b-419a-86c6-c158f0de660812 d agoJSON v1
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concepts[field].local:field:ocean-atmosphericmapping · data ucar educonnector:data_ucar_edu@1.0.0
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