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301.
D.-P. Häder P. Richter M. Schuster Ts. Dachev B. Tomov Pl. Georgiev Yu. Matviichuk 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Solar and space radiation have been monitored using the R3D-B2 radiation risks radiometer-dosimeter on board a recent space flight on the Russian satellite Foton M2 within the ESA Biopan 5 facility mounted on the outside of the satellite exposed to space conditions. The solar radiation has been assayed in four wavelength bands (UV-C, 170–280 nm, UV-B, 280–315 nm), UV-A (315–400 nm) and PAR (photosynthetic active radiation, 400–700 nm). The data show an increasing tumbling rotation of the satellite during the mission. The photodiodes do not show a cosine response to the incident light which has been corrected. After calibration of the signals using the extraterrestrial spectrum, doses have been calculated for each orbit, for each day and for the total mission as basic data for the biological material which has been exposed in parallel in the Biopan facility. Cosmic ionizing radiation has been monitored and separated in 256 deposited energy spectra, which were further used for determination of the absorbed dose rate and flux. Basic data tables were prepared to be used by other Biopan 5 experiments. The paper summarizes the results for the Earth radiation environment at the altitude (262–304 km) of the Foton M2 spacecraft. Comparisons with the predictions of NASA Earth radiation environment experimental models AE-8 and AP-8, and the PSB97 model are also presented, which calculate the fluxes of ionizing radiation from a simulation. AP-8 is a model for trapped radiation. 相似文献
302.
Pia Zacharias Sven Bingert Hardi Peter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
We study extreme-ultraviolet emission line spectra derived from three-dimensional magnetohydrodynamic models of structures in the corona. In order to investigate the effects of increased magnetic activity at photospheric levels in a numerical experiment, a much higher magnetic flux density is applied at the photosphere as compared to the Sun. Thus, we can expect our results to highlight the differences between the Sun and more active, but still solar-like stars. We discuss signatures seen in extreme-ultraviolet emission lines synthesized from these models and compare them to observed signatures in the spatial distribution and temporal evolution of Doppler shifts in lines formed in the transition region and corona. This is of major interest to test the quality of the underlying magnetohydrodynamic model to heat the corona, i.e. currents in the corona driven by photospheric motions (flux braiding). 相似文献
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直升机热管理与红外辐射特性耦合分析方法 总被引:1,自引:1,他引:0
未来高性能直升机面临提高能量利用率和抑制红外辐射特性的重大挑战,迫切需要协同解决这两个问题,需要从整机层面探究热管理和红外辐射特性耦合机制,建立耦合分析方法。直升机红外辐射特性不仅受到旋翼下洗流场、前飞流场和环境等外部因素的影响,还受到各子系统部件的工作状态、机身表面的散热口布置和红外抑制器的设计等热管理优化方法的影响。因此,直升机热管理问题和红外抑制问题是强相互耦合,必须统筹考虑。从直升机整机系统的结构特点、系统工作原理和能量平衡关系出发,基于热/质流产生、收集传输、储存利用和传热关系,分析直升机整机系统框架和传热平衡关系,建立以系统部件为内部边界条件、外环境为外部边界条件的整机耦合传热模型;通过对内外部热量的统筹调控与管理,提出热管理优化方法,实现既保障各系统安全高效工作、又提高整机能量利用率,优化红外辐射性能的目的。该模型和方法能为直升机综合热管理的方案设计和红外抑制方法提供支撑。 相似文献
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Qiumin Dai Xiande Fang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Solar radiation is one of the major factors that dominate the thermal behaviors of aerostats in the daytime and the primary energy source of high altitude long endurance aerostats. Therefore, it is necessary to propose an accurate model to predict the solar irradiances. A comprehensive review of the well-known solar radiation models is conducted to help develop the new model. Based on the analysis of the existing models and the available radiation data, the extensive computer tests of the regression and optimization are conducted, from which the new solar radiation model for direct and diffuse irradiances under clear sky conditions is proposed. The new model has excellent prediction accuracy. The coefficient of determination for direct radiation is 0.992, with the root mean square error (RMSE) of 16.9 W/m2 and the mean absolute error (MAE) of 2.2%. The coefficient of determination for diffuse radiation is 0.86, with RMSE = 8.7 W/m2 and MAE = 9.9%. Comparisons with the well-known existing models show that the new model is much more accurate than the best existing ones. 相似文献
310.
从某颗在轨卫星地面轨迹漂移“异常”出发,分析了该现象发生的内在机理,建立了零偏模式下(卫星姿态偏航角保持为零)光压摄动力沿迹方向累积效应解析模型,并基于历史观测数据通过轨道改进估计模型参数。最后,利用该卫星2018年真实地面轨迹对新模型预报精度进行验证。结果表明,采用新模型后,卫星地面轨迹漂移预报误差得到明显改善,为该卫星轨迹保持控制策略制定提供了技术支持。 相似文献