4.7 Article

Plasmapause location under quiet geomagnetic conditions (Kp ≤ 1): THEMIS observations

Journal

GEOPHYSICAL RESEARCH LETTERS
Volume 42, Issue 18, Pages 7303-7310

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1002/2015GL066090

Keywords

Plasmapause

Funding

  1. National Research Foundation (NRF) - Ministry of Education of Korea
  2. Basic Science Research Program through NRF [NRF-2013R1A1A2A10004414]
  3. Korea Polar Research Institute [PE15090]
  4. Div Atmospheric & Geospace Sciences
  5. Directorate For Geosciences [1101903] Funding Source: National Science Foundation
  6. Korea Institute of Marine Science & Technology Promotion (KIMST) [PE15090] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)

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We statistically examined the plasmapause location (L-pp) under quiet geomagnetic conditions (Kp1) using the electron density inferred from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft potential for 2year period (2008 and 2009). Five hundred forty-three L-pp samples were identified under steady quiet conditions with Kp values 1 during 12h prior to the plasmapause crossing. From our large data set, we determined the medians and means of L-pp in L and magnetic local time (MLT). They are located near geosynchronous orbit and nearly circular. The L-pp medians show a slight bulge located in postdusk sector. Comparing with previous models, our median or mean L-pp is extended approximate to 1-2L from the Earth than the model L-pp along the local time from 0800 to 2400 MLT. That is, L-pp locations in the previous models are underestimated during quiet geomagnetic conditions.

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