Volker Heesen is a staff scientist and radio astronomer at Hamburger Sternwarte with over a decade of experience studying radio continuum emission, cosmic-ray transport, and galactic magnetic fields. He has held postdoctoral positions at Southampton and Hertfordshire and earned a PhD from Ruhr University Bochum, focusing on polarimetric studies of edge-on galaxies. A member of LITTLE THINGS, LOFAR Magnetism and Surveys KSPs, and the JCMT NGLS, he combines observational expertise across LOFAR, VLA, and JCMT datasets. Volker is the author of Spinnaker, a 1-D cosmic-ray transport code used to model non-thermal radio spectral indices, reflecting his blend of software development and astrophysical modelling. Based in Hamburg, he brings a pragmatic, code-driven approach to probing how cosmic rays and magnetic fields shape galaxy evolution.
10 years of coding experience
7 years of employment as a software developer
Doctor of Philosophy (Ph.D.), Astronomy and Astrophysics, Doctor of Philosophy (Ph.D.), Astronomy and Astrophysics at Ruhr University Bochum
Master’s Degree, Physics, Master’s Degree, Physics at Technical University Munich
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Volker Heesen - Staff Scientist at University of Hamburg