FY-1C/D极轨气象卫星空间粒子成分监测器及其在轨探测结果

介绍了风云一号(FY-1)C，D极轨气象卫星空间粒子成分监测器的任务目标、主要功能和工程指标。以及数据的获取和处理方法。给出了空间环境宁静期、地磁扰动事件、太阳质子事件、与太阳活动的关系和粒子长期变化等探测结果，并进行了相应的分析。对C，D星空间粒子成分监测器分别进行的5年和第二次在轨测试结果表明，两星监测器工作正常、性能稳定，探测数据可靠。     

In situ dating on Mars: A new approach to the K–Ar method utilizing cosmogenic argon

Cosmogenic argon isotopes are produced in feldspars via nuclear reactions between cosmic rays and Ca and K atoms within the lattice. These cosmogenic isotopes can be used as proxies for K and Ca, much like nuclear reactor-derived ³⁹Ar and ³⁷Ar are used as proxies for K and Ca, respectively, in ⁴⁰Ar/³⁹Ar geochronology. If Ca and K are uniformly distributed, then the ratio of radiogenic ⁴⁰Ar (⁴⁰Ar^?) to cosmogenic ³⁸Ar or ³⁶Ar (³⁸Ar_cos or ³⁶Ar_cos) is proportional to the difference between the radioisotopic and exposure ages, as well as the K/Ca ratio of the degassing phase. Thus cosmogenic, radiogenic, and trapped Ar isotopes, all of which can be measured remotely and are stable over geologic time, are sufficient to generate an isochron-like diagram from which the isotopic composition of the trapped component may be inferred. Such data also provide a means to assess the extent to which the system has remained closed with respect to ⁴⁰Ar^?, thereby mitigating otherwise unquantifiable uncertainties that complicate the conventional K–Ar dating method.     

Shortcomings of the Standard Solar Model

The SSM, invented in early nineteen sixties, remains a useful construction. There are now much larger number of its predictions that may be compared with observations than when it was first introduced. Seismic sounding based on oscillations frequencies provides the best test of the physical input for modelling stellar evolution. The results of the test must be viewed as a support for the standard theory of stellar evolution. However, significant differences in the sound-speed, photospheric He abundance, and other parameters between the Sun and the current models remain. Shortcomings in the EOS and in treatment of convection have been revealed. The differences in the sound-speed in the radiative interior may be explained by small opacity errors but other explanations are possible. Results of seismic sounding support the idea that the element mixing in the outer part of the radiative interior occurred during a significant fraction of the Sun's life. Such mixing is considered as a possible explanation of the deficit of lithium. The shortcomings of SSM cannot explain the deficits of measured neutrino fluxes. This revised version was published online in June 2006 with corrections to the Cover Date.     

企业降低成本的有效途径

本文从产品价格是市场竞争的焦点出发，指出了企业降低成本的重要性。     

汽车发电机冷却风扇旋转噪声预测方法

以汽车发电机冷却风扇为对象,针对其修改叶片分布角度前后的旋转噪声预测问题,提出一套较精确且节约计算机时的预测方法.该方法结合了声类比法和矢量合成方法,首先,用大涡模拟(LES)和Ffowcs-Williams和Hawkings(FW-H)方程相结合的声类比方法对原风扇总噪声和主要阶次旋转噪声幅值进行预测;然后,针对只改变叶片分布角度情况下,提出一种矢量合成方法,用于对修改叶片分布前后主要阶次旋转噪声变化量的预测;最后,得到修改后主要阶次旋转噪声的幅值.计算和实验结果表明,原风扇总噪声最大预测误差4.3dB,第12阶和第18阶主要阶次旋转噪声幅值预测误差为1.24dB和4.26dB;修改后风扇第12阶和第18阶主要阶次旋转噪声分别变小了9.3dB和10.5dB,其变化量预测误差分别为0.36dB和0.43dB.结果表明,这一整套对修改前后风扇旋转噪声进行预测的方法是可行的,且大大节省计算时间,为风扇叶片周向分布角度设计提供了很好的依据.      

An updated model of atomic oxygen redline dayglow emission

A comprehensive model is developed using the updated rate coefficients and transition probabilities to study the redline dayglow emission of atomic oxygen. The solar EUV fluxes are obtained from the Solar Irradiance Platform (SIP), and incorporated into the model successfully. All possible production and loss mechanisms of O(¹D) are considered in the model. The neutral number densities and temperature are adopted from the NRLMSISE-00 model. The ion and electron densities, and electron temperature are adopted from the IRI-07 model. The model results are validated with the help of measurements as provided by the Wind Imaging Interferometer (WINDII) on board Upper Atmosphere Research Satellite (UARS). The present results are found in better agreement with the measurements in comparison with the earlier model. The measured volume emission rate profiles are reproduced quite well by the present model. The model results show that the updated rate coefficients and transition probabilities are quite consistent and may be used in the aeronomical studies.     

The high precision gamma-ray spectrometer for lunar polar orbiter SELENE

The high precision gamma-ray spectrometer (GRS) is scheduled to be launched on the lunar polar orbiter of the SELENE mission in 2007. The GRS consists of a large Ge crystal as a main detector and massive bismuth germanate crystals as an anticoincidence detector. A Stirling cryocooler was adopted in cooling the Ge detector. The flight model of SELENE GRS has been completed and an energy resolution of 3.0 keV (FWHM) at 1.332 MeV has been achieved. The spectrometer aims to observe nuclear line gamma rays emitted from the lunar surface in a wide energy range from 100 keV to 12 MeV for one year and more to obtain chemical composition on the entire lunar surface. The gamma-ray data enable us to study lunar geoscience problems including crust and mantle composition, and volatile reservoirs at polar regions.     

空间探测原子磁强计的主动磁补偿实验

在空间探测过程中,采用高灵敏无自旋交换弛豫(SERF)原子磁强计在行星表面进行磁场测量是原位物质成分分析的有效手段之一。为了提高SERF原子磁强计的磁场测量灵敏度,必须减小外界磁场扰动对其原子自旋SERF态质量的影响,基于SERF原子磁强计的测量原理,设计了一套主动磁补偿系统。首先,通过测量驱动激光光强获得3个方向的磁场信息;在此基础上,控制电流源和线圈主动产生一个与外界磁场扰动大小相同、方向相反的磁场来补偿扰动,以提高原子自旋SERF态的质量;最后,结合现有的SERF原子磁强计实验平台进行了实验验证。实验结果表明,与手动补偿方式相比,采用本文所述的主动磁补偿系统,可以实时跟踪磁场补偿点,降低系统信号的噪声,补偿了外界磁场的扰动,验证了磁强计主动磁补偿技术的有效性,为后续样机的研制奠定了技术基础。     

稀释氩气对分叉管内爆震波绕射的影响

为了研究稀释气体Ar的浓度对爆震波从直管往分叉管绕射传播和对直管中爆震波传播的影响,采用三阶TVD迎风格式和Strang-splitting算子分裂法,对H2/O2/Ar混合物爆震燃烧进行了二维数值计算。计算结果表明:在298K,6670Pa初始条件下,四种组分比条件下,主爆震管下游由于分叉管绕射稀疏波的影响,都会产生不同程度的解耦,但是通过壁面马赫反射后,都能恢复平面爆震;在H2/O2/Ar体积比为2:1:7时,爆震波绕射进入分叉管后,爆震波解耦成爆燃火焰波;体积比为2:1:0,2:1:1和2:1:4条件下,水平爆震管中的爆震波,绕射进入垂直分叉管后,通过不同次数壁面马赫反射,能够二次起爆,解耦的爆震波恢复成为平面自持爆震波。     

主成分分析法在宏观经济评价中的应用

文章主要介绍了主成分分析方法基本思想及其计算步骤,并用主成分分析方法在综合评价方面进行了实证分析,最后提出了在实际应用中应该注意的问题.