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We use coordinated Hinode SOT/EIS observations that include high-resolutionmagnetograms, chromospheric and TR imaging and TR/coronal spectra in a firsttest to study how the dynamics of the TR are driven by the highly dynamicphotospheric magnetic fields and the ubiquitous chromospheric waves. Initialanalysis shows that these connections are quite subtle and require acombination of techniques including magnetic field extrapolations,frequency-filtered time-series and comparisons with synthetic chromospheric andTR images from advanced 3D numerical simulations. As a first result, we findsignatures of magnetic flux emergence as well as 3 and 5 mHz wave power aboveregions of enhanced photospheric magnetic field in both chromospheric,transition region and coronal emission.

On connecting the dynamics of the chromosphere and transition region with Hinode SOT and EIS