Electrostatic reconnection in the ionosphere. Issue 6 (27th March 2015)

• Record Type: Journal Article
• Authors: Huba, J. D.; Wu, T.‐W.; Makela, J. J.
• Is Part Of: Geophysical research letters. Volume 42:Issue 6(2015:Mar.)
• Page Start: 1626
• Page End: 1631
• Publication Date: 2015-03-27
• Subjects: equatorial ionosphere -- equatorial spread F -- equatorial plasma bubbles -- equatorial dynamics -- electrostatic reconnection; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2015GL063187
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: Postsunset equatorial plasma bubble merging is examined using the National Research Laboratory code SAMI3/equatorial spread F . It is found that bubbles merge through an "electrostatic reconnection" process. As multiple bubbles develop, the electrostatic potential associated with one bubble can connect with that of a neighboring bubble: this provides a pathway for the low‐density plasma in one bubble to flow into the adjoining bubble and merge with it. Additionally, high‐speed plasma channels (approximately greater than hundreds of meters per second) can develop during the merging process. Optical data is presented of equatorial plasma bubble evolution that suggests bubble merging occurs in the nighttime equatorial ionosphere. Key Points: Plasma bubbles can merge in the nighttime equatorial ionosphere The merging process occurs by electrostatic reconnection Optical observations support the merging of equatorial plasma bubbles