Simultaneous longitudinal and transverse oscillations in filament threads after a failed eruption
Rakesh Mazumder, Vaibhav Pant, Manuel Luna, and Dipankar Banerjee

TL;DR
This study reports the simultaneous observation of longitudinal and transverse oscillations in a solar filament following a failed eruption, providing insights into the magnetic field and wave modes in filament threads.
Contribution
It presents the first simultaneous detection of both oscillation modes in a filament after a failed eruption, using AIA/SDO data and the pendulum model for magnetic field estimation.
Findings
Detected large amplitude longitudinal oscillations with damping.
Observed large amplitude transverse oscillations in a filament thread.
Estimated magnetic field strength and filament thread length from oscillation data.
Abstract
Longitudinal and transverse oscillations are frequently observed in the solar prominences and/or filaments. These oscillations are excited by a large scale shock wave, impulsive flares at one leg of the filament threads, or due to any low coronal eruptions. We report simultaneous longitudinal and transverse oscillations in the filament threads of a quiescent region filament. We observe a big filament in the north-west of the solar disk on July 2017. On July 2017 it starts rising around 13:00 UT. Then we observe a failed eruption and subsequently, the filament threads start to oscillate around 16 UT. We observe both transverse and longitudinal oscillations in a filament thread. The oscillations damp down and filament threads almost disappear. We place horizontal and vertical artificial slits on the filament threads to capture the longitudinal and transverse oscillations…
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