Ionospheric disturbances over Indonesia and their possible association with atmospheric gravity waves from the troposphere

被引:23
作者
Ogawa, Tadahiko [1 ]
Otsuka, Yuichi
Shiokawa, Kazuo
Saito, Akinori
Nishioka, Michi
机构
[1] Nagoya Univ, Solar Terrestrial Environm Lab, Toyokawa, Aichi 4428507, Japan
[2] Kyoto Univ, Grad Sch Sci, Dept Geophys, Kyoto, Japan
关键词
D O I
10.2151/jmsj.84A.327
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
As part of the CPEA (Coupling Processes in the Equatorial Atmosphere) project, we have been conducting ground-based optical and radio observations of the ionosphere and thermosphere at Kototabang in Indonesia, Japan, and Australia. First, this paper gives a brief overview of some results, paying special attention to 100-1000 km scale plasma disturbances in the F region ionosphere, i.e., medium-scale traveling ionospheric disturbances (MSTIDs) and plasma bubbles. MSTIDs over the equator are observed within and in the south of the F region equatorial anomaly crest and have, on the average, a phase velocity of 300 m s(-1) toward the south, a period of 40 min, and a wavelength of 700 km. Plasma bubbles move to the east at similar to 100 m s(-1), have a scale of about 100 km with spacings of 200-250 km, and are embedded within plasma structures with a scale of about 1000 km. Interestingly, giant plasma bubbles can be simultaneously detected at lower midlatitudes in southern and northern hemispheres that are connected by the geomagnetic field line, and are very identical in appearance in the both hemispheres. Then, we present newly-obtained characteristics of equatorial ionospheric scintillations of 1.6-GHz GPS radio waves associated with plasma bubbles. Continuous scintillation observations for two years at Kototabang indicate that the scintillations appear predominantly from sunset to midnight in equinoctial months. Such a seasonal variation is also recognized from a statistical study of bubble occurrences over the Philippines, Singapore, and Indonesia. To investigate possible dynamical coupling between the ionosphere/thermosphere and troposphere over the equator, we compare the scintillation (bubble) activity and Earth's brightness temperature variation over the Indian Ocean measured by meteorological satellites. The results indicate that there can exist meaningful correlations between the scintillation occurrence and tropospheric disturbance at 80 degrees-95 degrees E longitudes, i.e. 5 degrees-20 degrees west of Kototabang. Possible processes to seed plasma bubbles are discussed.
引用
收藏
页码:327 / 342
页数:16
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