Correlation between Poynting flux and soft electron precipitation in the dayside polar cap boundary regions. Issue 10 (27th October 2015)

• Record Type: Journal Article
• Authors: Deng, Yue; Sheng, Cheng; Su, Yi‐Jiun; Hairston, Marc R.; Knipp, Delores; Huang, Cheryl Y.; Ober, Daniel; Redmon, Rob J.; Coley, Robin
• Is Part Of: Journal of geophysical research. Volume 120:Issue 10(2015:Oct.)
• Page Start: 9102
• Page End: 9109
• Publication Date: 2015-10-27
• Subjects: cusp -- Poynting flux -- particle precipitation -- coincide -- Polar cap boundary -- dayside; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/2015JA021075
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: Observations have revealed large Poynting flux and soft electron precipitation around the cusp region, which have strong impacts on the polar ionosphere/thermosphere. Simulations also confirmed that Poynting flux and soft electron precipitation significantly change the neutral density and dynamics around the dayside polar cap boundary regions. However, no detailed study has been conducted to show if they should coincide with each other or not. Our analysis of Defense Meteorological Satellite Program (DMSP) satellite data reveals a complex correlation between them. Poynting flux and soft particle precipitation are coincident in some cases (match cases), but a clear displacement between them can also be identified in others (nonmatch cases). In the 29 cusp crossings from F13 we investigated, the ratio between nonmatch and match cases is close to 1:4. In nonmatch cases, the displacement between the Poynting flux enhancement and soft particle precipitation enhancement can be as large as 1° in geomagnetic latitude. Key Points: Correlation of Poynting flux and particle precipitation Relative location of two energy inputs in the dayside polar cap boundary Influence from the IMF conditions