التفاصيل البيبلوغرافية
| العنوان: |
Assessment of Polar Ionospheric Observations by VIPIR/Dynasonde at Jang Bogo Station, Antarctica: 2. Ionospheric Ion Drift Velocity. |
| المؤلفون: |
Kwon, Hyuck‐Jin, Jee, Geonhwa, Ham, Young‐Bae, Zabotin, Nikolay, Lee, Changsup, Kim, Ensol, Bullett, Terence W. |
| المصدر: |
Journal of Geophysical Research. Space Physics; May2024, Vol. 129 Issue 5, p1-11, 11p |
| مصطلحات موضوعية: |
ION migration & velocity, INCOHERENT scattering, GEOMAGNETISM, SOLAR cycle, CONSORTIA, ENERGY transfer, IONOSPHERE, DOPPLER effect, ECHO sounding |
| مصطلحات جغرافية: |
ANTARCTICA |
| مستخلص: |
Since the installation at the Antarctic Jang Bogo Station (JBS) in 2017, Korea Polar Research Institute (KOPRI) has been operating the Vertical Incidence Pulsed Ionospheric Radar (VIPIR) equipped with Dynasonde analysis (JVD). The two‐dimensional ion velocity is one of the key ionospheric parameters obtained from the JVD. The ionospheric ion velocities are compared with simultaneous, but independent, measurements of the Doppler velocity obtained from SuperDARN East radar at Dome C. The JVD ion velocity vector is projected to the line‐of‐sight direction of the SuperDARN observation over the JBS to be directly compared with each other. The result of comparison shows a reasonable agreement with the correlation coefficient of 0.72. The linear regression coefficient of about 0.5 represents that the JVD ion velocity is generally smaller than the SuperDARN observations by the regression coefficient, which may result from the different height ranges of the measurements. It is also found that the correlation coefficient increases with increasing magnetic activity (Kp), which suggests that the small‐scale ionospheric density irregularities tend to move with large‐scale plasma motion that is driven by enhanced plasma convection with increasing Kp. Plain Language Summary: The ion drift velocity in the polar ionosphere is one of the key parameters for understanding not only the dynamics of the ionosphere but also the magnetosphere‐ionosphere coupling processes and the magnetospheric energy transfer to the neutral atmosphere via ion‐neutral interactions. There are several ground‐based observational techniques to monitor the ion velocities in the polar region. For example, the incoherent scatter radars (ISRs) can determine the ion motion in the polar region, but usually require expensive resources for their maintenance and operation, which makes them affordable only to large organizations or international consortiums such as EISCAT. Another widely utilized observational system for the ion velocities in the polar region is the SuperDARN radars but they are relatively scarce in Antarctica. The most affordable technique for monitoring the ionosphere is the ionospheric sounding systems capable of observing not only the ionospheric densities but also the ion velocities in the bottomside ionosphere. An advanced sounding system has been operated at Jang Bogo Station in Antarctica since 2017 to produce ionospheric parameters including ion density and velocities. The observed ion velocities are compared with simultaneously observed SuperDARN ion velocities over the JBS and we discuss similarities and differences between the two measurements. Key Points: Validation of Dynasonde analysis (JVD) ion drift velocities by using simultaneous but independent SuperDARN observationsJVD ion velocities are generally in a good agreement with SuperDARN radar observationsSmall‐scale ionospheric density irregularities tends to move with large‐scale plasma contours as the geomagnetic activity increases [ABSTRACT FROM AUTHOR] |
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