The Strongest Magnetic Fields in the Universe / Space Sciences Series of ISSI Bd.54 (PDF)

Vasily Beskin is Professor and Senior Researcher at the Lebedev Physical Institute, Moscow, Russia. He is a leading theoretician in pulsar and neutron star physics. He is a member of the pulsar physics group at the Russian Academy of Sciences. He has published extensively on pulsar radiation mechanisms, formation and properties of radio pulsars and black hole magnetospheres. Among his publications one of the fundamental books is on the magnetohydrodynamics in compact astrophysical objects.

André Balogh, Professor Emeritus, Imperial College London, UK, is a renowned space physicist. He has been Director of the Space Physics Group at Imperial College and a Fellow of the American Geophysical Union, Royal Astronomical Society and European Geophysical Union. He has published several hundred peer-reviewed scientific papers in the leading journals of his field as author/co-author. He was PI on several space missions, in particular on the famous and successful CLUSTER mission. He has produced many successful students and PhDs. Among the books published by him are six co-edited SSSI-volumes and a monograph on Collisionless Shocks. He was a member of many scientific committees and is one of the leading figures in the investigation of near-Earth space.

Maurizio Falanga's scientific background is in high-energy astrophysics, mainly dealing with compact objects, and working as Science Program Manager at the International Space Science Institute. Since September 2013 he is Executive Director of the International Space Sciences Institute in Beijing, China, and Professor at the National Space Science Centre in Beijing, China. He has published over 100 papers in his research fields as author/co-author. At the same time, he has acted as supervisor for undergraduate and Ph.D. students.

Maxim Lyutikov, Professor at Purdue University, Indiana, USA, is a young theoretical physicist, astronomer and professor working in the high-energy astrophysical field. He