Large ion-neutral drift velocities and plasma heating in partially ionized coronal rain blobs
David Mart\'inez-G\'omez, Ram\'on Oliver, Elena Khomenko, Manuel, Collados

TL;DR
This study uses high-resolution 2D simulations to investigate ion-neutral drift velocities and plasma heating in partially ionized coronal rain blobs, revealing significant decoupling effects at the edges and associated temperature increases.
Contribution
First to demonstrate large ion-neutral drift velocities and temperature enhancements due to decoupling in coronal rain dynamics using a two-fluid model.
Findings
Strong coupling at the core with negligible drift velocities.
Weak coupling at the edges with drift velocities around 1 km/s.
Frictional heating causes temperature increases at the blob-corona boundary.
Abstract
In this paper we present a numerical study of the dynamics of partially ionized coronal rain blobs. We use a two-fluid model to perform a high-resolution 2D simulation that takes into account the collisional interaction between the charged and neutral particles contained in the plasma. We follow the evolution of a cold plasma condensation as it falls through an isothermal vertically stratified atmosphere that represents the much hotter and lighter solar corona. We study the consequences of the different degrees of collisional coupling that are present in the system. On the one hand, we find that at the dense core of the blob there is a very strong coupling and the charged and neutral components of the plasma behave as a single fluid, with negligible drift velocities (of a few cm s^-1). On the other hand, at the edges of the blob the coupling is much weaker and larger drift velocities…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Tropical and Extratropical Cyclones Research
