Propagation characteristics of Pi 2 pulsations observed at high- And low-latitude MAGDAS/CPMN stations: A statistical study

Teiji Uozumi, S. Abe, K. Kitamura, T. Tokunaga, A. Yoshikawa, H. Kawano, R. Marshall, R. J. Morris, B. M. Shevtsov, S. I. Solovyev, D. J. McNamara, K. Liou, S. Ohtani, M. Itonaga, K. Yumoto

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Abstract

The objective of this study is to understand better the propagation of Pi 2 waves in the nighttime region. We examined Pi 2 oscillations that showed high correlation between high- and low-latitude Magnetic Data Acquisition System/Circum Pan-Pacific Magnetometer Network stations (correlation coefficient: |γ| ≥ 0.75). For each horizontal component (H and D) we examined the magnetic local time (MLT) dependence of the delay time of high-latitude Pi 2 oscillations that corresponds to the highest correlation with the low-latitude Pi 2 oscillation. We found the delay time of the high-latitude H showed remarkable MLT dependence, especially in the premidnight sector: we found that in the premidnight sector the high-latitude H oscillation tends to delay from the low-latitude oscillation (<100 s). On the other hand, the delay time of the high-latitude D oscillation was not significant (∼±10 s) in the entire nighttime sector. We propose a Pi 2 propagation model to explain the observed delay time of high-correlation highlatitude H. The model quantitatively explains the trend of the event distribution. We also examined the spatial distribution of high-correlation Pi 2 events relative to the center of auroral breakups. It was found that the high-correlation Pi 2 events tend to occur away from the center of auroral breakups by more than 1.5 MLT. The present result suggests that the high-correlation H component Pi 2 oscillations at high latitude are a manifestation of forced Alfvén waves excited by fast magnetosonic waves.

Original languageEnglish
Article numberA11207
JournalJournal of Geophysical Research: Space Physics
Volume114
Issue number11
DOIs
Publication statusPublished - Nov 2009

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tropical regions
polar regions
Time delay
stations
oscillation
oscillations
propagation
time lag
sectors
Magnetometers
time dependence
Spatial distribution
Data acquisition
6-chloro-2-pyridylmethyl nitrate
station
correlation coefficients
magnetometers
data acquisition
spatial distribution
magnetometer

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

Cite this

Propagation characteristics of Pi 2 pulsations observed at high- And low-latitude MAGDAS/CPMN stations : A statistical study. / Uozumi, Teiji; Abe, S.; Kitamura, K.; Tokunaga, T.; Yoshikawa, A.; Kawano, H.; Marshall, R.; Morris, R. J.; Shevtsov, B. M.; Solovyev, S. I.; McNamara, D. J.; Liou, K.; Ohtani, S.; Itonaga, M.; Yumoto, K.

In: Journal of Geophysical Research: Space Physics, Vol. 114, No. 11, A11207, 11.2009.

Research output: Contribution to journalArticle

Uozumi, T, Abe, S, Kitamura, K, Tokunaga, T, Yoshikawa, A, Kawano, H, Marshall, R, Morris, RJ, Shevtsov, BM, Solovyev, SI, McNamara, DJ, Liou, K, Ohtani, S, Itonaga, M & Yumoto, K 2009, 'Propagation characteristics of Pi 2 pulsations observed at high- And low-latitude MAGDAS/CPMN stations: A statistical study', Journal of Geophysical Research: Space Physics, vol. 114, no. 11, A11207. https://doi.org/10.1029/2009JA014163
Uozumi, Teiji ; Abe, S. ; Kitamura, K. ; Tokunaga, T. ; Yoshikawa, A. ; Kawano, H. ; Marshall, R. ; Morris, R. J. ; Shevtsov, B. M. ; Solovyev, S. I. ; McNamara, D. J. ; Liou, K. ; Ohtani, S. ; Itonaga, M. ; Yumoto, K. / Propagation characteristics of Pi 2 pulsations observed at high- And low-latitude MAGDAS/CPMN stations : A statistical study. In: Journal of Geophysical Research: Space Physics. 2009 ; Vol. 114, No. 11.
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