Submitting Campus
Daytona Beach
Department
Physical Sciences
Document Type
Article
Publication/Presentation Date
6-18-2021
Abstract/Description
This study exploits the volumetric sampling capabilities of the Resolute Bay Incoherent Scatter Radar (RISR-N) in collaboration with all-sky imagery and in-situ measurements (DMSP) to examine the interplay between cold plasma transport and auroral precipitation during a high-latitude lobe reconnection event on the dawn side. The IMF had an impulsive negative excursion in B$_z$ embedded within a prolonged period of B$_z>0$ and B$_y
Publication Title
Journal of Geophysical Research - Space Physics
DOI
https://doi.org/10.1002/essoar.10507316.1
Publisher
Wiley
Grant or Award Name
NSF grant ATM 544 1821135, NSF AGS-1255181 and NASA NNX14AQ39G, NASA grants 80NSSC18K0657, 80NSSC20K0604 and 80NSSC20K0725, NSF grant 551 AGS-1907698, and AFOSR grant FA9559-16-1-0364
Scholarly Commons Citation
Pena, J. D., Semeter, J., Nishimura, Y., Varney, R., Reimer, A., Hairston, M., Zettergren, M., Hirsch, M., Verkhoglyadova, O., Hosokawa, K., & Shiokawa, K. (2021). Auroral Heating of Plasma Patches Due to High-Latitude Reconnection. Journal of Geophysical Research - Space Physics, (). https://doi.org/10.1002/essoar.10507316.1
