3D simulations of supernova remnants evolution including non-linear particle acceleration
Federico Fraschetti | Lunar and Planetary Laboratory & Department of Planetary Sciences | The University of Arizona
Efficient turbulent amplification of magnetic field driven by dynamo effect at supernova remnant shocks
Proton Beams of Death - Jeremy J. Drake
Federico FRASCHETTI | The University of Arizona, Arizona | UA | Department of Planetary Sciences
Federico Fraschetti - FCC - JRC FotoCineClub
5 "Federico Fraschetti" profiles | LinkedIn
Federico Fraschetti (@FredUS76) / Twitter
University of Arizona | Planetary Science AND ASTRONOMY - Academia.edu
arXiv:1909.04092v1 [astro-ph.SR] 9 Sep 2019
Federico Fraschetti
arXiv:0809.3686v1 [astro-ph] 22 Sep 2008
Ultra-high-energy cosmic rays from the radio lobes of active galactic nuclei
arXiv:1808.04812v1 [astro-ph.SR] 14 Aug 2018
Federico Fraschetti - FCC - JRC FotoCineClub
Federico FRASCHETTI | The University of Arizona, Arizona | UA | Department of Planetary Sciences
Federico Fraschetti
Federico Fraschetti (@FredUS76) / Twitter
The Tenth Marcel Grossmann Meeting : GENERAL FEATURES OF GRB 030329 IN THE EMBH MODEL
FEDERICO FRASCHETTI
arXiv:1002.5048v2 [astro-ph.HE] 1 Jul 2010
Simonetta Fraschetti
Powerful particles and tugging tides may affe | EurekAlert!
