Observations of instability-driven nanojets
A. Ramada C. Sukarmadji, Patrick Antolin, James A. McLaughlin

TL;DR
This study presents IRIS and SDO observations of nanojets in the solar corona, revealing their association with magnetic reconnection driven by instabilities like KHI and RTI, and highlighting their widespread occurrence.
Contribution
It provides the first detailed observational evidence of nanojets across different coronal structures and identifies the dynamic instabilities responsible for their formation.
Findings
Nanojets are accompanied by nanoflare-like intensity bursts.
Nanojets have velocities of 150-250 km/s and occur transversely to magnetic field lines.
Kelvin-Helmholtz and Rayleigh-Taylor instabilities are identified as drivers.
Abstract
The recent discovery of nanojets by Antolin et al. (2021) represents magnetic reconnection in a braided field, thus clearly identifying the reconnection-driven nanoflares. Due to their small scale (500 km in widths, 1500 km in lengths) and short timescales ( 15 s), it is unclear how pervasive nanojets are in the solar corona. In this paper, we present IRIS and SDO observations of nanojets found in multiple coronal structures, namely in a coronal loop powered by a blowout jet, and in two other coronal loops with coronal rain. In agreement with previous findings, we observe that nanojets are accompanied by small nanoflare-like intensity bursts in the (E)UV, have velocities of 150-250 km s and occur transversely to the field line of origin, which is sometimes observed to split. However, we find a variety of nanojet directions in the plane transverse to the loop axis. These…
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Taxonomy
TopicsCentral Venous Catheters and Hemodialysis · Streptococcal Infections and Treatments · Seismic Waves and Analysis
