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131.
Noraset Wichaipanich Pornchai Supnithi Mamoru Ishii Takashi Maruyama 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
In this paper, the F2-layer critical frequency (foF2) and peak height (hmF2) measured by the FM/CW ionosonde at Thailand equatorial latitude station, namely Chumphon (10.72°N, 99.37°E, dip 3.22) are presented. The measurement data during low solar activity from January 2004 to December 2006 are analyzed based on the diurnal, seasonal variation. The results are then compared with IRI-2001 model predictions. Our study shows that: (1) In general, both the URSI and CCIR options of the IRI model give foF2 close to the measured ones, but the CCIR option produces a smaller range of deviation than the URSI option. The agreement during daytime is generally better than during nighttime. Overestimation mostly occurs in 2004 and 2006, while underestimation is during pre-sunrise hours in June solstice in 2005. The peak foF2 around sunset is higher during March equinox and September equinox than the other seasons, with longer duration of maximum levels in March equinox than September equinox. Large coefficients of variability foF2 occur during pre-sunrise hours. Meanwhile, the best agreement between the observed foF2 and the IRI model is obtained in June solstice. (2) In general, The IRI (CCIR) model predicts the observed hmF2 well during daytime in June solstice from 2004–2006, but it overestimates during March equinox, September equinox and December solstice. For nighttime, the model overestimates hmF2 values for all seasons especially during March equinox and September equinox. However, the model underestimates hmF2 values during September equinox and for some cases during June solstice and December solstice at pre-sunrise. The agreement between the IRI model and the hmF2(M3000OBS) is worst around noontime, post-sunset and pre-sunrise hours. All comparative studies give feedback for new improvements of CCIR and URSI IRI models. 相似文献
132.
Tiju Joseph Mathew S.R. Prabhakaran Nayar Sudha Ravindran Tarun Pant 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Post-sunset and pre-sunrise vertical plasma drifts at the equatorial F-region have been investigated using the HF Doppler radar and ionosonde observations. Observed vertical plasma drift features during the sunrise are found to complement that observed during the evening. The post-sunset vertical plasma drift is characterized by an upward enhancement, a pre-reversal enhancement and a reversal in the drift direction. Similarly, the pre-sunrise plasma drift is characterized by a sudden downward excursion followed by an upward turning. The wavelet analysis of the plasma drift shows the presence of fluctuations in the period range 4–32 min and the short period fluctuations are attributed to the atmospheric gravity waves. 相似文献
133.
L.A. McKinnell M.W. Paradza P.J. Cilliers M.A. Abdu J.R. de Souza 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The probability of occurrence of spread-F can be modeled and predicted using neural networks (NNs). This paper presents a feasibility study into the development of a NN based model for the prediction of the probability of occurrence of spread-F over selected equatorial stations within the Brazilian sector. The input space included the day number (seasonal variation), hour (diurnal variation), sunspot number (measure of the solar activity), magnetic index (measure of the magnetic activity) and magnetic position. Twelve years of spread-F data from Brazil (covering the period 1978–1989) measured at the equatorial site Fortaleza (3.9°S, 38.45°W) and low latitude site Cachoeira Paulista (22.6°S, 45.0°W) are used in the development of an input space and NN architecture for the model. Spread-F data that is believed to be related to plasma bubble developments (range spread-F) was used in the development of the model. The model results show the probability of spread-F occurrence as a function of local time, season and latitude. Results from the Brazilian Sector NN (BSNN) based model are presented in this paper, as well as a comparative analysis with a Brazilian model developed for the same purpose. 相似文献
134.
Sanjay Kumar A.K. Singh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The ionospheric total electron content (TEC), derived by analyzing dual frequency signals from the Global Positioning System (GPS) recorded near the Indian equatorial anomaly region, Varanasi (geomagnetic latitude 14°, 55′N, geomagnetic longitude 154°E) is studied. Specifically, we studied monthly, seasonal and annual variations as well as solar and geomagnetic effects on the equatorial ionospheric anomaly (EIA) during the solar minimum period from May 2007 to April 2008. It is found that the daily maximum TEC near equatorial anomaly crest yield their maximum values during the equinox months and their minimum values during the summer. Using monthly averaged peak magnitude of TEC, a clear semiannual variation is seen with two maxima occurring in both spring and autumn. Statistical studies indicate that the variation of EIA crest in TEC is poorly correlated with Dst-index (r = −0.03) but correlated well with Kp-index (r = 0.82). The EIA crest in TEC is found to be more developed around 12:30 LT. 相似文献
135.
概要介绍了外逸电子发射机理,综述了国内外外逸电子研究概况、水平趋势及在各个领域的应用,并结合表面特性、疲劳特点,剂量测量和计数管等,试图为飞机机翼、火车道轨等金属材料的无损检测,开拓一条新的途径。 相似文献
136.
对大气中声重波的产生源的效率作了分析计算。结果显示,不同源的效率相差很大,而且还随频率、离原的距离和方向,以及不同的波动参量而变。对于极光带电急流产生声重波的源,即洛伦兹力和焦耳加热两个源来说,产生近场声重波的效率以洛伦兹为高、对于沿极光带电急流平面的运场区声重波而言,焦耳加热的效率高得多。但对垂直于极为带电流平面的速度波动则洛伦兹力的产生效率高得多;对于沿极光带电急流平面的法向的远场区内的所有声重波参量而言,洛地兹力的产生效率高得多。 相似文献
137.
本文给出了1983-1985年磁暴期间,我国乌鲁木齐等七个站及日本国分寺等五个站出现微粒E层的情况;得到了微粒E层的日变化、月变化和纬度变化;结合同时的地磁、宇宙线、TEC和电离层的变化,对微粒E层出现率作了分析。初步证实:微粒E层的形成和维持与赤道环电流指数(Dst)负变幅大小密切相关,此外还同宇宙线的FD(Forbushdecreases)事件的出现有关。作者认为,沉降粒子可能是低纬地区微粒E层事件的主要粒子来源。 相似文献
138.
本文研究了高频寻常波在均匀等离子体中垂直均匀背景磁场传播时,由于在传播方向上有限区域内存在等幅密度扰动驻波引起共振折反射的理论.认为这种共振反射理论可能解释ESF条件下VHF/UHF雷达强散射和卫星与地面通讯中断等现象. 相似文献
139.
140.
《北京航空航天大学学报》2012,38(8)
基于宽行加工理论和广域曲率吻合原则,提出一种利用圆环面内侧作为刀具工作面的反圆环面刀具宽行加工叶片进排气边的新方法.该方法通过优化刀具摆角使具有定母圆半径刀具工作面的包络面充分逼近叶片进排气边曲面,从而使刀具能在给定的精度范围内以最大行宽和最少刀轨行数加工出进排气边.最后,以某型号发动机叶片的进气边为例进行了加工实验.结果表明该方法能够大幅提高进排气边的加工质量,且反圆环面刀的加工行宽比球头刀提高了5倍. 相似文献