DOI QR코드

DOI QR Code

Characteristics of the Polar Ionosphere Based on the Chatanika and Sondrestrom Incoherent Scatter Radars

  • Kwak, Young-Sil (Department of Astronomy and Atmospheric Science, Kyungpook National University) ;
  • Ahn, Byung-Ho (Department of Earth Science, Kyungpook National University)
  • Published : 2004.09.30

Abstract

The climatological characteristics of the polar ionospheric currents obtained from the simultaneous observations of the ionospheric electric field and conductivity are examined. For this purpose, 43 and 109 days of measurements from the Chatanika and Sondrestrom incoherent scatter radars are utilized respectively. The ionospheric current density is compared with the corresponding ground magnetic disturbance. Several interesting characteristics about the polar ionosphere are apparent from this study: (1) The sun determines largely the conductance over the Sondrestrom radar, while the nighttime conductance distribution over the Chatanika radar is significantly affected by auroral precipitation. (2) The regions of the maximum N-S electric field over the Chatanika radar are located approximately at the dawn and dusk sectors, while they tend to shift towards dayside over the Sondrestrom radar. The N-S component over Son-drestrom is slightly stronger than Chatanika. However, the E-W component over Chatanika is negligible compared to that of Sondrestrom. (3) The E-W ionospheric current flows dominantly in the night hemisphere over Chatanika, while it flows in the sunlit hemisphere over Sondrestrom. The N-S current over Chatanika flows prominently in the dawn and dusk sectors, while a strong southward current flows in the prenoon sector over Sondrestrom. (4) The assumption of infinite sheet current approximation is far from realistic, underestimating the current density by a factor of 2 or more. It is particularly serious for the higher latitude region. (5) The correlation between ${\Delta}H\;and\;J_E$ is higher than the one between ${\Delta}D\;and\;J_N$, indicating that field-aligned current affects ${\Delta}D$significantly.

Keywords

References

  1. Ahn, B.-H., B.A. Emery, H.W. Kroehl, and Y. Kamide. 1999. Climatological characteristics of the auroral ionosphere in terms of electric field and ionospheric conductance conductance. J. Geophys. Res., 104, 10031-10040. https://doi.org/10.1029/1999JA900043
  2. Araki, T., K. Schlegel, and H. Luhr. 1989. Geomagnetic effects of the Hall and Pedersen current flowing in the auroral ionosphere. J. Geophys. Res., 94, 17185-17199. https://doi.org/10.1029/JA094iA12p17185
  3. Barton, C.E. 1997. International geomagnetic reference field: The seventh generation. J. Geomag. Geoelectr., 49, 123-148. https://doi.org/10.5636/jgg.49.123
  4. Brekke, A., J.R. Doupnik, and P.M. Banks. 1974. Incoherent scatter measurement of E region conductivities and current in the auroral zone. J. Geophys. Res., 79, 3773-3790. https://doi.org/10.1029/JA079i025p03773
  5. Chapman, S. and J. Bartels. 1940. Geomagnetism, Vol. 1. Clarendon, Oxford.
  6. Hedin, A.E. 1991. Extension of the MSIS thermospheric model into the middle and lower atmosphere. J. Geophys. Res., 82, 2851-2853. https://doi.org/10.1029/JA082i019p02851
  7. Iijima, T. and T.A. Potemra. 1976. The amplitude distribution of field-aligned currents at northern high latitude observed by TRIAD. J. Geophys. Res., 81, 2165-2174. https://doi.org/10.1029/JA081i013p02165
  8. Kamide, Y. and A. Brekke. 1975. Auroral electrojet current density deduced from the Chatanika radar and from the Alaska meridian chain of magnetic observatories. J. Geophys. Res., 80, 587-594. https://doi.org/10.1029/JA080i004p00587
  9. Kamide, Y., S.-I. Akasofu, and A. Brekke. 1976. Ionosphere current obtained from the Chatanika radar and ground magnetic perturbations at the auroral latitude. Planet. Space Sci., 24, 173-201.
  10. Kamide, Y., W. Sun, and S.-I. Akasofu. 1996. The average ionospheric electrodynamics for the different substorm phases. J. Geophys. Res., 101, 99-109. https://doi.org/10.1029/95JA02990
  11. Popov, V.A., V.O. Papitashvili, and J.F. Watermann. 2001. Modeling of equivalent ionospheric currents from meridian magnetometer chain data. Earth Planets Space, 53, 129-137. https://doi.org/10.1186/BF03352370
  12. Tanskanen, E.I., A. Viljanen, T.I. Pulkkinen, R. Pirjola, L. Häkkinen, A. Pulkkinen, and O. Amm. 2001. At substorm onset, 40% of AL comes from underground. J. Geophys. Res., 106, 13119-13134. https://doi.org/10.1029/2000JA900135