In this joint talk, we will provide an overview of plasma physics research in the context of space and astrophysical environments, charting a journey from our local heliosphere to distant compact objects. We will begin by covering the fundamentals of heliospheric plasmas, including the physics of the solar corona, the properties of the solar wind, and the dynamics of near-Earth plasmas [1]. We...
Astrophysical jets are highly collimated outflows observed in a wide range of astronomical systems, from young stellar objects and X-ray binaries to active galactic nuclei (AGN). These jets are intimately linked to the accretion processes occurring around forming stars or supermassive black holes at the centers of galaxies. I will focus on the extragalactic case, where jets are accelerated to...
I will discuss the main plasma physics challenges to understand how particles scatter inside their acceleration region, around their sources and in the medium between the source and the observer. I will outline how non-linear process are expected to play a crucial role in all of these cases and their phenomenological implications.
X-ray synchrotron radiation is expected to be highly polarized. Thanks to the Imaging X-ray Polarimetry Explorer (IXPE), it is now possible to evaluate the degree of X-ray polarization in sources such as supernova remnants (SNRs). Jointly using IXPE data and high-resolution Chandra observations, we perform a spatially resolved spectropolarimetric analysis of SNR Cassiopeia A (Cas A). We focus...
