most citedCan We Improve the Preprocessing of Photospheric Vector Magnetograms by the Inclusion of Chromospheric Observations?

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astro-ph2008★ 63 cited

Can We Improve the Preprocessing of Photospheric Vector Magnetograms by the Inclusion of Chromospheric Observations?

T. Wiegelmann, J. K. Thalmann, C. J. Schrijver +2

The solar magnetic field is key to understanding the physical processes in the solar atmosphere. Nonlinear force-free codes have been shown to be useful in extrapolating the corona…

astro-ph2006

F-mode sensitivity kernels for flows

J. Jackiewicz, L. Gizon, A. C. Birch

We compute f-mode sensitivity kernels for flows. Using a two-dimensional model, the scattered wavefield is calculated in the first Born approximation. We test the correctness of th…