The Siberian Solar Radio Telescope: the current state of the instrument,observations, and data

The Siberian Solar Radio Telescope (SSRT) is one of the world's largest solar radio heliographs. It commenced operation in 1983, and since then has undergone several upgrades. The operating frequency of the SSRT is 5.7 GHz. Since 1992 the instrument has had the capability to make one-dimensional scans with a high time resolution of 56 ms and an angular resolution of 15 arc sec. Making one of these scans now takes 14 ms. In 1996 the capability was added to make full, two-dimensional images of the solar disk. The SSRT is now capable of obtaining images with an angular resolution of 21 arc sec every 2 min. In this paper we describe the main features and operation of the instrument, particularly emphasizing issues pertaining to the imaging process and factors limiting data quality. Some of the data processing and analysis techniques are discussed. We present examples of full-disk solar images of the quiet Sun, recorded near solar activity minimum, and images of specific structures: plages, coronal bright points, filaments and prominences, and coronal holes. We also present some observations of dynamic phenomena, such as eruptive prominences and solar flares, which illustrate the high-time-resolution observations that can be done with this instrument. We compare SSRT observations at 5.7 GHz, including computed `light curves', both morphologically and quantatively, with observations made in other spectral domains, such as 17 GHz radio images, Hα filtergrams and magnetograms, extreme-ultraviolet and X-ray observations, and dynamic radio spectra.     

The investigation of the solar wind transsonic region at meter wavelengths

Radio astronomy experiments designed to probe the interplanetary plasma close to the Sun have been carried out at the wavelength = 2.92 m using the occultation method. The experiments are based on a modification of the occultation method by which the sources, in this case quasars, are used to measure the radial dependence of the apparent source size, the scattering angle (R). The radial dependence of this source size (R) reveals that an anomalous enhancement in the scattering appears at radial distances from about 16 to 30 R , which is associated with the solar wind transsonic region. It is shown by analysis of the theoretical equations that the radial profiles of both the source size (R) and the scintillation index m(R) are consistent in the near solar interplanetary medium (R 40 R ). Combining these two independent applications of the occultation method extends the range of the investigation and provides a powerful new diagnostic of the solar wind transsonic region.     

火试金法测定铜精矿中金含量结果的不确定度评定

对火试金法测定铜精矿中金含量的结果进行不确定度评定。分析了铜精矿样品称量、铜精矿样品的不均匀性和配料处理,以及金粒称量等因素对金含量测量结果不确定度的影响,并得出火试金法测量铜精矿中金含量的扩展不确定度。     

某型短波电台的中频数字化设计

针对短波射频数字化对器件的要求较高,功耗较大,现在一般采用中频数字化技术.给出了某型短波电台的中频数字化设计方案,介绍了电台中频数字化部分的实现方法及基本原理.并介绍了本设计中使用的Inters公司生产的数字上变频器HSP50415,美国AD公司生产的数字接收信号处理芯片AD6620和TI公司TMS320VC5416芯片的结构、功能和特点,给出了它们在数字变频应用的硬件模块接口图.测试结果证明,通过在中频部分使用数字变频器提高了电台的收发性能,较模拟化中频有着成本低廉、功耗低、兼容性好和可扩展性好.     

扎赉诺尔坳陷带砂体特征及找铀矿方向分析

扎赉诺尔坳陷带内诸凹陷具有不同的沉积特征和砂体特点,查干诺尔和克鲁伦凹陷砂体形成于粗粒冲积扇和扇三角洲沉积体系,砂体厚度变化大,相变快,有机质含量低,顶底板均不发育;呼伦湖凹陷以小型三角洲平原相砂体为主,具有较稳定的泥砂岩结构,有机质含量高,砂体厚度和横向延伸较稳定,但砂体铀含量较低;胡列也吐凹陷砂体以辫状河三角洲体系产出为主,砂体厚度大,延伸稳定,底板发育,顶板发育不完全,砂体铀含量高.扎赉诺尔坳陷带各凹陷砂体的不同特点,决定了它们具有不同的找矿潜力.通过砂体综合条件对比分析,笔者认为胡列也吐凹陷和克鲁伦凹陷砂体铀成矿条件较好,呼伦湖凹陷次之,查干诺尔凹陷较差.     

Characteristics of Scour and Deposition in Front of Breakwaters Under Irregular Broken Clapotis

First the scour and deposition patterns of the sandy seabed in front of a vertical breakwater under the action of irregular broken clapotis are investigated experimentally and classified into five types: scour type Ⅰ , scour type Ⅱ, scour type Ⅲ, deposition type Ⅰ, and deposition type Ⅱ . Secondly, the processes of formation of scour and deposition patterns are probed in comparison with those induced by regular broken clapotis and standing waves. Thirdly, the criteria for distinguishing scour and deposition patterns under irregular broken clapotis are presented.     

扇贝肝胰腺化学成分的初步研究

通过多种化学分析方法 ,初步探讨了扇贝肝胰腺组织的化学成分。结果表明 :该组织中含有较丰富的营养物质 ,并含有重要生理活性的 EPA和 DHA,微量元素含量也很丰富。这些结果为扇贝加工后下脚料的利用 ,提供了基础资料     

乳糖诱导重组别藻蓝蛋白(rAPC)在大肠杆菌(Escherichia coli)中的表达

采用廉价的乳糖替代IPTG诱导重组别藻蓝蛋白(rAPC)在大肠杆菌(Escherichiacoli)JM109中表达,对诱导产物表达的培养基、培养条件、诱导剂的浓度和诱导时机进行了优化,将优化条件用于5L自控发酵罐进行高密度培养。结果表明,对rAPC表达的条件进行优化后,乳糖诱导rAPC的表达率可达26.8%,与IPTG的诱导结果接近;在高密度培养中,OD600最大达21.8。研究结果可为乳糖替代IPTG大规模生产rAPC奠定基础。     

Analysis of solutions to the inverse problem on the retrieval of the microstructure of stratospheric aerosol from satellite measurements

A statistical ensemble of microphysical parameters of the background stratospheric aerosol at altitudes of 15 to 30 km is modeled on the basis of experimental data. The aerosol attenuation coefficients (AACs) in the wavelength range 0.38–16.3 μm are calculated for all realizations of the ensemble by algorithms of the Mie theory. Analysis of correlations between the AACs and the microphysical parameters indicate that the AAC correlates most strongly with the total volume V and area S of all particles. The errors of determining the microphysical parameters from AAC measurements are analyzed via the method of linear regression. It is shown that, if the AAC is measured with an error of 5%, the errors of determining both the particle size distribution (PSD) for particles with sizes of 0.4 to 4 μm and the parameter S are an order of magnitude smaller than the prior uncertainty, whereas the error of determining V is two orders of magnitude smaller than the prior uncertainty. Schemes of AAC measurements with the SAGE III, ISAMS, CLAES, HALOE instruments and an IR interferometer in the visible and IR regions are discussed. It is shown that combining the schemes makes it possible to extend the range of particle sizes for which the PSD is retrieved with a satisfactory accuracy and to increase the accuracy of determining S and V substantially and the accuracy of determining the total number of particles N _opt to a lesser extent. Examples of interpreting AAC measurements carried out simultaneously with the SAGE III and HALOE instruments within the same spatial region are presented. A systematic discrepancy between vertical profiles of S and V obtained from SAGE III and HALOE measurements is revealed.