An Automated Algorithm for Identifying and Tracking Transverse Waves in Solar Images
Micah J. Weberg, Richard J. Morton, and James A. McLaughlin

TL;DR
This paper introduces an automated algorithm for detecting and analyzing transverse waves in solar images, enabling large-scale statistical studies of wave properties crucial for understanding solar atmospheric dynamics.
Contribution
The paper presents a novel automated method for identifying and tracking transverse waves in solar images, validated with synthetic data and applied to real observations, improving analysis speed and accuracy.
Findings
Algorithm achieves 1-2% accuracy in displacement amplitudes
Wave periods and velocities measured with 4-10% accuracy
35-41% of observed plumes show multiple wave signatures
Abstract
Recent instrumentation has demonstrated that the solar atmosphere supports omnipresent transverse waves, which could play a key role in energizing the solar corona. Large-scale studies are required in order to build up an understanding of the general properties of these transverse waves. To help facilitate this, we present an automated algorithm for identifying and tracking features in solar images and extracting the wave properties of any observed transverse oscillations. We test and calibrate our algorithm using a set of synthetic data which includes noise and rotational effects. The results indicate an accuracy of 1-2% for displacement amplitudes and 4-10% for wave periods and velocity amplitudes. We also apply the algorithm to data from the Atmospheric Imaging Assembly (AIA) on board the (SDO) and find good agreement with previous studies. Of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
