Übersicht der Projekte am KIS

CASSDA: The CASSDA project - Centre for Advanced Solar Spectro-polarimetric Data Analysis - is conceived to provide to the solar physics community with accurate spectroscopic and spectro-polarimetric datasets observed at the German telescopes.
EAST - EST: The European Association for Solar Telescopes (EAST) was founded in 2006 by a group of solar physicists from 14 European countries. The goal of EAST is to ensure access of European solar astronomers to world-class high-resolution ground-based observing facilities.
HotMol: This project develops several exploratory theoretical and observational aspects of precision spectropolarimetry for detecting water vapour and other volatiles on exoplanets and in the inner part of protoplanetary disks.
InnoPol: Polarimetry is a powerful technique for revealing two- and three-dimensional structures in astrophysical objects beyond the spatial resolution provided by direct imaging at any telescope.
ORIGIN: The core of this project is to gain insight in the processes that are of major relevance for the solar dynamo by novel and improved methods of helioseismology. The analyses go far beyond the state-of-the-art and are based on highly resolved velocity measurements on the Sun from NASA’s milestone missions SOHO and SDO as well as the instruments of the GONG network.
SOLARNET: SOLARNET brings together and integrates the major European research infrastructures in the field of high-resolution solar physics, in order to promote their coordinated use and development.
SolarOrbiter PHI-ISS: Solar Orbiter ist eine ESA Mission zur Beobachtung der Sonne bei hoher räumlicher Auflösung und für in-situ Messungen der Heliosphäre sehr nahe der Sonne.
SpaceInn: The European Helio- and Asteroseismology Network (HELAS) has initiated the project "Exploitation of Space Data for Innovative Helio- and Asteroseismology - SpaceInn" with the mission to build on the existing European strength in the field of time-domain stellar physics.
Sunrise: Sunrise ist ein ballongetragenes Sonnenteleskop mit einer Öffnung von einem Meter. Es wird die Sonne im sichtbaren und nah-ultravioletten Licht beobachten (400 bis 215 nm).
Visible Tunable Filter: The Visible Tunable Filter (VTF) for the Daniel K. Inouye Solar Telescope is an imaging spectro-polarimeter for the wavelength range between 520 and 860 nm. It operates at the highest spatial resolution possible for the DKIST, 20 km on the Sun, equivalent to an angular resolution of 0.028 arcseconds.