Speaker
Ignasi J. Soler Poquet
(Rosseland Centre for Solar Physics, University of Oslo, Norway)
Description
AtLAST observations at (sub-)millimeter wavelengths of the full solar disk will provide complementary perspectives on our Sun. The combination of simultaneous observation across a wide frequency range [from 30 to 950 GHz] at full polarisation states, the high temporal evolution, and the production of synoptic maps, will offer a new view of the solar atmosphere. These specifications will facilitate AtLAST to address a wide range of scientific topics including the thermal structure and heating of the solar chromosphere, flares and prominences, and the solar activity cycle
Author
Ignasi J. Soler Poquet
(Rosseland Centre for Solar Physics, University of Oslo, Norway)