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- W2007054095 abstract "We observed weak magnetic flux in enhanced Ca K network and in its surroundings at various positions on the solar disc ($costheta=1.0dots0.1$). The Gregory Coude Telescope at the Observatorio del Teide on Tenerife was used together with an image scanner and a Stokes V polarimeter. ${1over2}(I_lambdapm V_lambda)$ spectrograms in the 6302 A region were taken. A second order flat fielding and smoothing brought the polarimetric sensitivity to a detection limit of 0.001 $I_mathrm{c}$ (with $I_mathrm{c}$ = continuum intensity) for exposure times of 300 ms in pixels corresponding to 0$farcs$ $5times$0$farcs$19 ($widehat=$ slit width $times$ pixel size of detector). We present correlations between continuum intensity, line center intensity, and magnetic flux and discuss Stokes V profiles. The V amplitude asymmetry from areas with strong flux decreases towards the limb, a change of sign is not identified. The magnetic fields are ordered around strong flux centers with decreasing mean field strength outwards from the centers. In the range of $1times 10^{16}$ Mx to $5times 10^{16}$ Mx (in one pixel of $5times 10^{14}$ cm 2 ) the probability distribution of the magnetic flux is ~$|Phi|^{-q}$ with $qapprox3$, different from a Gaussian distribution. From this we derive tentativily a radial dependence from the flux centers of the form $Phi(r)sim1/r$. For the probability distributions a significant center-to-limb variation is not detected. Together with the center-to-limb behaviour of the asymmetries, we interpret this tentatively as an isotropic orientation of the weak magnetic flux elements and of the gas flows. A vertical orientation of the magnetic fields is also compatible with the measurements, though." @default.
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- W2007054095 date "2002-04-01" @default.
- W2007054095 modified "2023-09-25" @default.
- W2007054095 title "Weak magnetic flux features on the Sun" @default.
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- W2007054095 doi "https://doi.org/10.1051/0004-6361:20020081" @default.
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