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在分析对比现有的雷达罩设计方法基础上,针对某型直升机机栽雷达罩,研究了雷达罩设计过程中的基本问题、关键技术和综合优化设计方法,运用三维射线追踪法进行了计算机辅助设计,给出了布设防雷击部件的经验公式,讨论了吸波材料选择与喷涂的基本准则。电测结果表明:加罩后的功率传输系数、反射瓣、雷达辐射特性等指标的实测数据与计算值符合较好,满足了设计要求。 相似文献
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电磁波从宇宙空间对地传输过程中,不可避免需要穿过地球电离层,并受到电离层折射、反射、穿透等影响。为研究电离层中电磁波的传播路径,利用IRI2016电离层模型和NRLMSISE-00模型的数据,基于射线追踪算法,综合利用龙格-库塔法,并采用变步长实现了电磁波在电离层多层空间复杂等离子体中的传输计算。同时,还研究了不同频率和纬度的电磁波在电离层的传播途径。研究表明较高频率的电磁波受到电离层的干扰较少,在100MHz时,电磁传播的偏移角度仅为0.795度;电离层的非均匀层状结构决定了电磁波在其中的传输存在多模现象,并受到了光照的影响,在日间和中纬均受电离层的强烈干扰,偏移角度均大于2.2度,较夜间和低、高纬地区的传输偏移更大。 相似文献
117.
M. Sasaki S. Haino K. Abe H. Fuke T. Hams K.C. Kim M.H. Lee Y. Makida S. Matsuda J.W. Mitchell A.A. Moiseev J. Nishimura M. Nozaki S. Orito J.F. Ormes T. Sanuki E.S. Seo Y. Shikaze R.E. Streitmatter J. Suzuki K. Tanaka T. Yamagami A. Yamamoto T. Yoshida K. Yoshimura 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
In this paper, we report searches for antihelium in cosmic rays using two recently flown magnetic rigidity spectrometers. BESS-TeV had extended rigidity with an MDR of 1.4 TV and had a flight duration of one day. BESS-Polar was optimized for collecting power. It was flown for 8.5 days and had an MDR of 240 GV. The former flight allows us to explore a previously unexplored rigidity band and the latter flight yields a factor of three improvement in the overall BESS limit. No antihelium candidate was found in the rigidity ranges of 1–500 GV, and 0.6–20 GV, among 7 × 104 events taken with BESS-TeV, and 8 × 106 events taken with BESS-Polar, respectively. 相似文献
118.
M. Papailiou H. Mavromichalaki A. Vassilaki K.M. Kelesidis G.A. Mertzanos B. Petropoulos 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
There is an increasing amount of evidence linking biological effects to solar and geomagnetic disturbances. A series of studies is published referring to the changes in human physiological responses at different levels of geomagnetic activity. In this study, the possible relation between the daily variations of cosmic ray intensity, measured by the Neutron Monitor at the Cosmic Ray Station of the University of Athens (http://cosray.phys.uoa.gr) and the average daily and hourly heart rate variations of persons, with no symptoms or hospital admission, monitored by Holter electrocardiogram, is considered. This work refers to a group of persons admitted to the cardiological clinic of the KAT Hospital in Athens during the time period from 4th to 24th December 2006 that is characterized by extreme solar and geomagnetic activity. A series of Forbush decreases started on 6th December and lasted until the end of the month and a great solar proton event causing a Ground Level Enhancement (GLE) of the cosmic ray intensity on 13th December occurred. A sudden decrease of the cosmic ray intensity on 15th December, when a geomagnetic storm was registered, was also recorded in Athens Neutron Monitor station (cut-off rigidity 8.53 GV) with amplitude of 4%. It is noticed that during geomagnetically quiet days the heart rate and the cosmic ray intensity variations are positively correlated. When intense cosmic ray variations, like Forbush decreases and relativistic proton events produced by strong solar phenomena occur, cosmic ray intensity and heart rate get minimum values and their variations, also, coincide. During these events the correlation coefficient of these two parameters changes and follows the behavior of the cosmic ray intensity variations. This is only a small part of an extended investigation, which has begun using data from the year 2002 and is still in progress. 相似文献
119.
利用地面宇宙线强度变化预报地磁暴方法初步研究 总被引:1,自引:0,他引:1
分析了Nagoya宇宙线闪烁体望远镜探测数据的变化特点,定性地探讨了CME可能引起的地面宇宙线的变化特征,通过实例证实了地面宇宙线通量的异常波动是地磁暴发生的重要先兆特征,并且将8 h内宇宙线通量与该时间段内平均通量的偏差D8(t)参数应用到宇宙线数据分析中.通过数据分析与讨论,认为D8(t)参数达到一定阈值是地磁暴的重要先兆特征,但不是充分条件,虚假信号仍占多数;D8(t)参数与太阳质子事件探测结果相结合,对于大地磁暴的预报有较好的效果. 相似文献
120.
Rajesh K. Mishra Rekha Agarwal Mishra 《空间科学学报》2007,27(5):353-359
In the present work the cosmic ray intensity data recorded with ground-based neutron monitor at Deep River has investigated taking into account the associated interplanetary magnetic field and solar wind plasma data during 1981—1994.A large number of days having abnormally high/low amplitudes for successive number of five or more days as compared to annual average amplitude of diurnal anisotropy have been taken as high/low amplitude anisotropic wave train events(HAE/LAE).The amplitude of the diurnal anisotropy of these events is found to increase on the days of magnetic cloud as compared to the days prior to the event and it found to decrease during the later period of the event as the cloud passes the Earth.The High-Speed Solar Wind Streams(HSSWS)do not play any significant role in causing these types of events. The interplanetary disturbances(magnetic clouds)are also effective in producing cosmic ray decreases.Hαsolar flares have a good positive correlation with both amplitude and direction of the anisotropy for HAEs, whereas PMSs have a good positive correlation with both amplitude and direction of the anisotropy for LAEs. The source responsible for these unusual anisotropic wave trains in CR has been proposed. 相似文献