The dynamics of the solar radiative interior are still poorly constrained by comparison to the convective zone. This disparity is even more marked when we...

We describe the design of the Sunrise Filter Imager (SuFI) and the Image Stabilization and Light Distribution (ISLiD) unit onboard the Sunrise balloon borne...

The main properties of the first- and second-order moments of polarized hydrogen lines, forming in the presence of stationary electric and magnetic fields, are...

The Global Oscillation Network Group (GONG) Project will place a network of instruments around the world to observe solar oscillations as continuously as...

SUNRISE III is a balloon-borne solar observatory dedicated to investigating the physics governing the magnetism and dynamics in the lower solar atmosphere. The...

The Imaging Magnetograph eXperiment (IMaX) is a spectropolarimeter built by four institutions in Spain that flew on board the Sunrise balloon-borne solar...

With the steady improvement of the observing capabilities and numerical simulations, an efficient data management of large data volumes has become mandatory...

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The development of effective iterative methods capable of accurately solving NLTE Stokes transfer problems is of considerable importance for the investigation...