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首页> 外文期刊>Earth, planets and space: EPS >Equatorial GPS ionospheric scintillations over Kototabang, Indonesia and their relation to atmospheric waves from below
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Equatorial GPS ionospheric scintillations over Kototabang, Indonesia and their relation to atmospheric waves from below

机译:印度尼西亚科托邦的赤道GPS电离层闪烁及其与来自下方的大气波的关系

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摘要

Using Global Positioning System (GPS) satellites. we have been conducting equatorial ionospheric scintillation observations at Kototabang, Indonesia since January 2003. Scintillations caused by equatorial plasma bubbles appear between 2000 and 0 100 LT in equinoctial months with a seasonal asymmetry, and their activity decreases with decreasing solar activity. A comparison between scintillation index (S-4) and Earth's brightness temperature variations suggests that file scintillation activity call be related to tropospheric disturbances over file Indian Ocean to the west of Kototabang. TO Understand better the reasons of day-to-day variability of S-4, we analyze S-4. T-bb and lower thermospheric neutral wind ((mu'(2)) over bar) data. The results show that S-4 fluctuates with periods of about 2.5, 5, 8, 14 and 25 days, possibly due to atmospheric waves from below and that similar periods are also found in the T-bb and (mu'(2)) over tilde variations. Using a general circulation model, we made numerical simulations to determine the behavior of neutral wind in the equatorial thermosphere. The results indicate the following: (1) 2- to 20-day waves dissipate rapidly above about an altitude of 125 km, and 0.5- to 3-hour waves become predominant above 100 km, (2) zonal winds above 200 km altitude are, on the whole, eastward during sunset-sunrise, (3) zonal wind patterns due to short-period (1-4 h) atmospheric gravity waves (AGWs) above 120 km altitude change day by day, exhibit wavy structures with scale lengths of about 30-1000 km and, as it whole, move eastward in about 100(-1) while changing patterns over time. These simulations suggest that the Rayleigh-Taylor instability responsible for plasma bubble generation call be seeded by AGWs with short periods of about 0.5-3 h, and that background conditions necessary for this instability are modulated by planetary-scale atmospheric waves propagating up to an altitude of about 120 km front below.
机译:使用全球定位系统(GPS)卫星。自2003年1月以来,我们一直在印度尼西亚科托邦(Kototabang)进行赤道电离层闪烁观测。由赤道等离子体气泡引起的闪烁出现在季节不对称的等月数2000到0 100 LT之间,并且其活动随着太阳活动的减少而降低。闪烁指数(S-4)与地球亮度温度变化之间的比较表明,文件闪烁活动的发生与科托班邦以西印度洋的对流层扰动有关。为了更好地了解S-4日常变化的原因,我们分析了S-4。 T-bb和较低的热层中性风((bar上的(mu'(2)))数据。结果表明,S-4的周期大约为2.5、5、8、14和25天,这可能是由于来自下方的大气波引起的,并且在T-bb和(mu'(2))中也发现了类似的周期波浪号变化。使用通用循环模型,我们进行了数值模拟,以确定赤道热圈中性风的行为。结果表明:(1)2至20天的海浪在125 km左右的高度以上迅速消散,而0.5至3小时的海浪在100 km以上的高度中占主导地位,(2)200 km以上的纬向风总体而言,在日落-日出期间向东,(3)海拔120 km以上的短周期(1-4 h)大气重力波(AGW)引起的纬向风型逐日变化,呈现出波浪状结构,尺度长度为大约30-1000公里,并且整体上会向东移动约100(-1),同时会随着时间的推移而变化。这些模拟表明,引起等离子气泡产生的瑞利-泰勒不稳定性是由短时长约0.5-3 h的AGW播种的,而这种不稳定性所必需的背景条件是由传播到一个高度的行星尺度大气波调制的下方约120公里处

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