Young, Peter R., Viall, Nicholeen M., Kirk, Michael S., Mason, Emily I. and Chitta, Lakshmi Pradeep (2021) An Analysis of Spikes in Atmospheric Imaging Assembly (AIA) Data. Solar Physics, 296 (12). p. 181. ISSN 0038-0938
|
Text
Young2021_Article_AnAnalysisOfSpikesInAtmospheri.pdf - Published Version Available under License Creative Commons Attribution 4.0. Download (4MB) | Preview |
Abstract
The Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) returns high-resolution images of the solar atmosphere in seven extreme ultraviolet (EUV) wavelength channels. The images are processed on the ground to remove intensity spikes arising from energetic particles hitting the instrument, and the despiked images are provided to the community. In this article, a three-hour series of images from the 171 Å channel obtained on 28 February 2017 was studied to investigate how often the despiking algorithm gave false positives caused by compact brightenings in the solar atmosphere. The latter were identified through spikes appearing in the same detector pixel for three consecutive frames. 1096 examples were found from the 900 image frames. These “three-spikes” were assigned to 126 dynamic solar features, and it is estimated that the three-spike method identifies 19% of the total number of features affected by despiking. For any ten-minute sequence of AIA 171 Å images there are around 37 solar features that have their intensity modified by despiking. The features are found in active regions, quiet Sun, and coronal holes and, in relation to solar surface area, there is a greater proportion within coronal holes. In 96% of the cases, the despiked structure is a compact brightening with a size of two arcsec or less, and the remaining 4% have narrow, elongated structures. By applying an EUV burst detection algorithm, we found that 96% of the events could be classified as EUV bursts. None of the spike events are rendered invisible by the AIA processing pipeline, but the total intensity over an event’s lifetime can be reduced by up to 67%. Users are recommended to always restore the original intensities in AIA data when studying short-lived or rapidly evolving features that exhibit fine-scale structure.
| Item Type: | Article |
|---|---|
| Additional Information: | Funding Information: We acknowledge support from NASA’s Heliophysics Guest Investigators program and the GSFC Internal Scientist Funding Model competitive work package program. E.I. Mason’s research was supported by an appointment to the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by the Universities Space Research Association under contract with NASA. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 695075). |
| Uncontrolled Keywords: | Corona: quiet, Coronal holes, Jets, Instrumental effects, Cosmic rays: solar |
| Subjects: | F300 Physics F500 Astronomy |
| Department: | Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering |
| Depositing User: | John Coen |
| Date Deposited: | 12 Jan 2022 13:55 |
| Last Modified: | 12 Jan 2022 14:00 |
| URI: | http://nrl.northumbria.ac.uk/id/eprint/48144 |
Actions (login required)
 |
View Item |
Downloads
Downloads per month over past year
