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1.
本文用自制的装有 BaF_2探头的高探测效率的正电子湮没寿命谱仪测量了在室温下正电子素 o-Ps 与 p-RPhG 及 m-RPhG(R=NO_2,Cl,H,CH_3,cH_3O)在20%(V/V)二氧六环水溶液中的络合形成速度常数。实验结果表明,这些o-Ps-M 络合形成速度常数 K 值均与作为配位体的 p-RPhG、m-RPhG 的碱性解离常数 K 的负对数 pK_2 呈线性函数。这表明上述瞬态络合反应满足线性自由能关系,由此可推断出上述络合反应的一些重要性质。 相似文献
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Changlong Jiang Jianping Xiong Xugang Zhang Huibo Jia Duanyi Xu 《Aerospace and Electronic Systems Magazine, IEEE》2003,18(11):31-34
Most sustained data recording systems in many real-time fields are based on tape equipments. We have developed an innovative sustained data recording system based on disk array which consists of Array Controller Module (ACM), String Controller Module (SCM) and Main Controller Module (MCM). This system has a better performance and higher reliability than the traditional tape recorder and can be used conveniently in many areas of data recording, storing, playback, and remote backup. This novel recording system has been used in radar data recorder for spacecraft orbit tracking and satellite remote sensing data recording successfully. 相似文献
3.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,39(5):661-667
Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with hourly time interval resolution for the diurnal variation, obtained with DPS-4 digisonde observations at Hainan (19.4°N, 109.0°E) are used to study the low latitude ionospheric variation behavior. The observational results are compared with the International Reference Ionospheric Model (IRI) predictions. The time period coverage of the data used for the present study is from March 2002 to February 2005. Our present study showed that: (1) In general, IRI predictions using CCIR and URSI coefficients follow well the diurnal and seasonal variation patterns of the experimental values of foF2. However, CCIR foF2 and URSI foF2 IRI predictions systematically underestimate the observed results during most time period of the day, with the percentage difference ΔfoF2 (%) values changing between about −5% and −25%, whereas for a few hours around pre-sunrise, the IRI predictions generally overestimate the observational ones with ΔfoF2 (%) sometimes reaching as large as ∼30%. The agreement between the IRI results and the observational ones is better for the year 2002 than for the other years. The best agreement between the IRI results and the observational ones is obtained in summer when using URSI coefficients, with the seasonal average values of ΔfoF2 (%) being within the limits of ±10%. (2) In general, the IRI predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the observational results. However, when using the measured M(3000)F2 as input, the diurnal variation pattern of hmF2 given by IRI2001 has a much better agreement with the observational one with the detailed fine structures including the pre-sunrise and post-sunset peaks reproduced reasonably well. The agreement between the IRI predicted hmF2 values using CCIR M(30,000)F2 option and the observational ones is worst for the afternoon to post-midnight hours for the high solar activity year 2002. During daytime hours the agreement between the hmF2 values obtained with CCIR M(30,000)F2 option and the observational ones is best for summer season. The discrepancy between the observational hmF2 and that obtained with CCIR M(30,000)F2 option stem from the CCIR M(3000)F2 model, which does not produce the small scale structures observed in the measured M(3000)F2. 相似文献
4.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(10):1846-1850
Emissions from solar flares may reveal fast fluctuations, which can be attributed to small-scale injections of energetic electrons. In this paper, we perform numerical calculations of the Hα emission from a flaring atmosphere bombarded by a pulsating electron beam. We assume that the variation of the electron beam flux consists of two components: a fluctuation component and a background component. The results show that the amplitude of Hα fluctuations varies depending on the magnitude of the background flux of the electron beam. In the case of a higher background flux, the Hα fluctuations are more significant than in the case of a lower background flux. This result is compatible with the observations in which the Hα fluctuations appear preferentially near the hard X-ray maximum. 相似文献
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《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1986,6(8):243-251
The Coronal Helium Abundance Spacelab Experiment (CHASE) was designed and built in the UK by groups at the Rutherford Appleton Laboratory and at the Mullard Space Science Laboratory. The main objective of the experiment was to improve the measurement of the abundance of helium in the Sun, which currently is uncertain by a factor of approximately three. Since most of this helium must be of primordial origin, being formed within a few minutes of the big bang, such a measurement would also have significant cosmological implications.The instrument consisted of a grazing incidence telescope feeding a 1200 lines mm−1 diffraction grating. Parts of the dispersed spectrum were then observed around the Rowland circle with channel electron multipliers and a channel multiplier array plate. During the flight, good observations were made of the Lyman-α lines of hydrogen at 1216 A and of ionised helium at 304 A, both in the corona, where the lines are formed by resonance scattering, and on the solar disc where excitation of the lines is much more complex.The spectrometer was also able to observe many other transition region and coronal lines in ions of O, S and Fe. Images in these lines clearly show how the magnetic fields in active regions constrain the material in arch-shaped loops with the hot material towards the top. 相似文献
8.
When Bioregenerative Life Support System (BLSS) is used for long-term deep space exploration in the future, it is possible to perform closed-loop control on growth of microalgae to effectively regulate O2 production process in emergencies. However, designing controller of microalgae cultivating device (MCD) by means of traditional methods is very difficult or even impossible due to its highly nonlinearity and large operation scope. In our research, the Artificial Neural Network Model Reference Control (ANN-MRC) method was therefore utilized for model identification and controller design for O2 production process of a specific MCD prototype—photo bioreactor (PBR), based on actual experiment and computer simulation. The results demonstrated that the ANN-MRC servo controller could robustly and self-adaptively control and regulate the light intensity of PBR to make O2 concentrations in vent pipe be in line with step reference concentrations with prescribed dynamic response performance. 相似文献
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10.
程俊兰 《北华航天工业学院学报》2007,17(3):9-11
目前,小内存的数控机床仍然是我国机床的主流,使加工程序变得简洁,对实际加工有着很重要的意义.宏程序的应用可以大大简化编程,本文通过实例介绍了数控铣削加工外球面的宏程序. 相似文献