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931.
932.
O.S. Oyekola 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Measurements of the critical frequency, foF2 recorded over Ibadan: 7.4°N, 3.9°E (geographic), 6°S (dip angle) have been compared with the International Reference Ionosphere (IRI-2007) model for solar maximum geomagnetically quiet conditions, with a view to determining what modifications might bring about better predictions for the model. Our results reveal that the present version of IRI essentially reproduces diurnal trends and the general features of the experimental observations for all seasons, except for nighttime June solstice periods, which the model seriously overestimated. The model errors ranging from 50% to 125% over the four seasons considered in this study. It is also indicated that the percentage relative deviations between the observed and the modeled values vary approximately from −11% to 12% (March), −34% to 11% (June), −16% to 12% (September), and −10% to 13% (December). An unexpected feature of foF2 is obvious and remarkable reduction in values during nighttime June solstice periods compared to that in other seasons. Relationship between equatorial vertical drift and foF2 is also investigated. However, cross correlation analysis reveals strong anti-correlation between vertical drift and critical frequency during the daytime hours, but exceptionally opposite is the case for the nighttime sector. The discrepancies which are noted, particularly during June solstice season are attributed to processes most likely within the thermosphere and from meteorological influences during quiet magnetic conditions. 相似文献
933.
R.U. Beisembaev V.I. Drobzhev E.A. Dryn O.N. Kryakunova N.F. Nikolaevskiy 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Ground level enhancements of cosmic ray intensity registered by means of neutron monitors at middle latitudes were studied by using Student’s criterion. Three of these events on 6 November 1997, 24 August 1998, and 13 December 2006 were analyzed in detail. It is shown that the use of Student’s criterion allows revealing effectively the ground level enhancements at middle latitudes. 相似文献
934.
935.
针对因卫星入境数据延迟,无法快速判断太阳能电池阵温度遥测数据是否发生异常问题,提出一种SE-TCN网络模型。首先借鉴SENet中的通道注意力机制,对时间卷积网络(TCN)进行改进,提高模型的特征提取能力;其次使用SE-TCN做为特征提取网络,训练出网络模型;最后对温度遥测数据做中长期预测(约4轨)。以某在轨卫星实际太阳能电池阵温度遥测数据作为实验数据。结果表明:本文提出的SE-TCN网络模型在评价指标上与传统TCN网络模型相比,平均绝对误差(MAE)降低了7.7%,均方根误差(RMSE)降低了5.2%,相关系数(R)提高了0.4%。当卫星入境时,该检测方法可根据预测值快速判断实时遥测数据是否发生异常。 相似文献
936.
937.
F3 layer feature under low and medium solar activity observed at a Chinese low latitude station Fuke
Zhengping Zhu Kun Chen Jiaping Lan Fenglou Sun 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Ionogram observations from the ionosonde at Fuke (9.5°N geomagnetic latitude), a Chinese low latitude station, in 2010–2012 are analyzed to present the features of F3 layer under low and moderate solar activity conditions. Structure of the ionogram, displaying the F3 layer, was more distinct and clear during MSA than LSA periods especially during spring to summer. Start time of occurrence of the F3 layer is about at 0830–0900 LT and is approximately the same for LSA and MSA conditions. The average duration time of the F3 layer occurrence was 181 min per day under F10.7 = 75 condition, 263 min in F10.7 = 99 and 358 min in F10.7 = 125, respectively. The differences of h′F2 and h′F3 exhibited obvious semiannual variation observed at Fuke from March 2010 to June 2012 and increased with increasing solar activity. The difference of foF2 and foF3 in the months February, March, September, October and November is less evident in the middle solar activity period 2011–2012 than the low solar activity 2010 and in the other period it shows a slight increase (0.5 MHz) or keeps constant. The results show that the solar activity dependence of the F3 layer occurrence at low latitude away from the magnetic equator is different from that at near the magnetic equator. 相似文献
938.
939.
940.
Giannina Poletto 《Space Science Reviews》1994,70(1-2):241-252
Streamers have been observed since far back in time, but our knowledge of their morphology and of their physical characteristics is still very limited. As a consequence, the present streamer picture is largely incomplete: because individual features are poorly known, their role in more general phenomena (like the evolution of the global corona or the solar wind mass and flow pattern) is also poorly known. In this presentation, the more relevant open problems in the understanding of streamers will be illustrated and it will be shown how new data acquired by SOHO may help us to reach a better understanding of these structures. 相似文献