Atomic and Ionized Microstructures in the Diffuse Interstellar Medium
Snezana Stanimirovic, Ellen G. Zweibel (University of Wisconsin,, Madison)

TL;DR
This review discusses small-scale atomic and ionized structures in the interstellar medium, emphasizing their physical properties, origins, and significance for understanding turbulence and energy processes in space.
Contribution
It synthesizes observational and theoretical insights into AU-scale microstructures, proposing they result from turbulent cascades and local energy sources.
Findings
Microstructures are linked to turbulent dissipation scales.
Evidence suggests both universal turbulence and discrete origins.
Microstructures are associated with supernova remnants and local bubbles.
Abstract
It has been known for half a century that the interstellar medium (ISM) of our Galaxy is structured on scales as small as a few hundred km, more than 10 orders of magnitude smaller than typical ISM structures and energy input scales. In this review we focus on neutral and ionized structures on spatial scales of a few to ~10^4 Astronomical Units (AU) which appear to be highly overpressured, as these have the most important role in the dynamics and energy balance of interstellar gas: the Tiny Scale Atomic Structure (TSAS) and Extreme Scattering Events (ESEs) as the most over-pressured example of the Tiny Scale Ionized Structures (TSIS). We review observational results and highlight key physical processes at AU scales. We present evidence for and against microstructures as part of a universal turbulent cascade and as discrete structures, and review their association with supernova…
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