Nettsider med emneord «USA»
The ClimFun project, funded by the Research Council of Norway, will increase our understanding about how fungi respond to global change.
The Swedish 1-m Solar Telescope (SST) on La Palma is the world leading facility for high resolution observations of the Sun.
Mapping the universe from the Milky Way to the Big Bang
The project is a ground-based CMB polarization experiment observing from the Atacama desert in Chile.
Instabilities and turbulence in the polar ionosphere studied with the integrated, multi-scale 4D (3D in space and time) experimental, theoretical, and modelling approach.
Nuclear physics has as its objective the investigation and understanding of nuclei, which are the hearts of atoms and the place where almost all mass of visible matter resides. The rules of nuclear binding determine the number of stable isotopes and their relative abundance in the world we live. Nuclei are fermion systems comprising from a few to hundred of neutrons and protons. The systems are small enough to exhibit sharp quantum states, but also large enough to show collective degrees of freedom, like vibrations and rotations.
Bringing together evolution and ecology through the Red Queen Perspective
The LIPCHEM group combines synthetic organic chemistry, medicinal chemistry and total organic synthesis to study the chemistry and biology of lipids, particularly metabolites of the omega-3 fatty acids eicosapentaenoic acid (EPA) and docosahexaenoic acid (DHA).
The Research Council of Norway has funded the project “Vortex flows and magnetic tornadoes on the Sun and cool stars” for the period 2013 to 2017. The aim of the VORTEX project is the comprehensive study of vortex flows and magnetic tornadoes on the Sun and other stars.
The SolarALMA project was funded with a Consolidator Grant by the European Research Council (ERC) and ran from September 2016 to August 2021. The aim was to utilise the first observations of the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA), which promises significant steps towards understanding the outer layers of the solar atmosphere with possible contributions to solving the coronal heating problem.