Ionospheric measurements of relative coronal brightness during the total solar eclipses of 11 August, 1999 and 9 July, 1945

Swept-frequency (1/10 MHz) ionosonde measurements were made at Helston, Cornwall (50°06N, 5°18W) during the total solar eclipse on August 11, 1999. Soundings were made every three minutes. We present a method for estimating the percentage of the ionising solar radiation which remains unobscured at any time during the eclipse by comparing the variation of the ionospheric E-layer with the behaviour of the layer during a control day. Application to the ionosonde date for 11 August, 1999, shows that the flux of solar ionising radiation fell to a minimum of 25±2% of the value before and after the eclipse. For comparison, the same technique was also applied to measurements made during the total solar eclipse of 9 July, 1945, at Sörmjöle (63°68N, 20°20E) and yielded a corresponding minimum of 16 ± 2%. Therefore the method can detect variations in the fraction of solar emissions that originate from the unobscured corona and chromosphere. We discuss the differences between these two eclipses in terms of the nature of the eclipse, short-term fluctuations, the sunspot cycle and the recently-discovered long-term change in the coronal magnetic field.     

基于光合有效辐射的西北太平洋柔鱼资源丰度和空间分布变动研究

光合有效辐射(PAR)对于海洋初级生产力具有显著的调控作用,会间接影响到头足类的资源丰度和渔场分布。本文根据2006−2015年上海海洋大学鱿钓科学技术组提供的柔鱼鱿钓数据和光合有效辐射卫星遥感数据,研究了光合有效辐射与西北太平洋柔鱼种群的关系,并评估了异常环境条件下光合有效辐射对柔鱼的影响。结果发现,柔鱼单位捕捞努力量渔获量(CPUE)、渔场纬度重心、PAR,及其空间分布均具有显著的月间变化。7−11月各月适宜PAR范围分别为36～39 E/(m²·d)、33～36 E/(m²·d)、24～27 E/(m²·d)、18 E/(m²·d)和12 E/(m²·d),最适宜PAR值分别为36 E/(m²·d)、33 E/(m²·d)、27 E/(m²·d)、18 E/(m²·d)和12 E/(m²·d)。此外,CPUE与PAR有显著正相关关系(p<0.05),且CPUE与各月适宜PAR范围占渔场比例也呈显著正相关(p<0.05);同时渔场纬度重心随各月最适PAR平均纬度变化而变化。在异常环境条件下,拉尼娜年份CPUE值比厄尔尼诺年份高,该年份PAR值异常增高可能是导致柔鱼资源丰度增加的因素之一。研究表明,光合有效辐射对于西北太平洋柔鱼资源丰度和空间分布具有显著影响。     

用于太阳紫外辐射测量传感器的设计

介绍了太阳紫外辐射的测量原理,为了提高入射光学系统的余弦响应特性而设计的余弦漫射器,以及等效辐射平面位置的计算方法。设计了适用于海滨浴场等场所的太阳紫外线辐射传感器的光学系统结构,研制了试验样机,开展了相应的试验,并对试验结果进行了分析。     

EXPERIMENTAL STUDY ON EFFECTS OF HUMIDITY AND CHEMICAL COMPOSITION UPON IMAGINARY PART OF REFRACTIVE INDEX OF AEROSOL PARTICLES*

Experimental study is made of the relationship between the imaginary part of refractive index (IRI) of atmospheric aerosol particles and relative humidity,and between IRI and chemical element through the assay of chemical constituents of the particles.Evidence suggests that atmospheric humidity and aerosols' chemical ingredients have great effects on the IRI's and they should thus be considered in the research of the radiation properties of the particles in the atmosphere.     

Analytical evaluation of the relativistic thermodynamic functions using binomial expansion theorem and incomplete Gamma functions

A simple evaluation algorithm for calculation of the fermions and bosons relativistic thermodynamic functions with high accuracy is presented. This method is based on the use of the binomial expansion theorems and incomplete Gamma functions. The importance of this result is that it enables a series analytical formula to determine the thermodynamic functions of fermions and bosons in cases of degeneracy and relativity. The formulas obtained are numerically stable for ψ < 0. Examples of comparative calculations are given. Numerical results verify the effectiveness of the present approach and they are in good agreement with literature.     

Phenomenological explanation for the shape of the spectrum of cosmic rays with energies <Emphasis Type="Italic">E</Emphasis> > 10 GeV

Assuming that the energy gain by cosmic-ray (CR) particles is a stochastic process with stationary increments, we derive expressions for the shape of their energy spectrum up to energies E ～ 10¹⁸ eV. In the ultrarelativistic case under study, the energy is proportional to the momentum, whose time derivative is the force. According to the Fermi mechanism, a particle accelerates when it passes through a system of shock waves produced by supernova explosions. Since these random forces act on time scales much shorter than the particle lifetime, we assume them to be delta-correlated in time. In this case, due to the linear energy-momentum relationship, the mean square of the energy (increments) is proportional to the differential scale τ(E) ～ Eτ(≥E), where τ (≥E) is the cumulative time it takes for a particle to gain an energy ≥E. The probability of finding a particle with energy ≥E somewhere in the system is inversely proportional to the time it takes to gain the energy E. To estimate an upper limit for the space number density of CR particles, we use estimates of the CR volume energy density, a quantity known for our Galaxy. It is taken to be constant in the range 10 GeV ≤ E ≤ 3 × 10⁶ GeV, where the index of the energy spectrum was found to be ?8/3 ≈ ?2.67 against its empirical value of ?2.7. In the range 3 × 10⁶ GeV ≤ E < 10⁹ GeV, the upper limit for the volume energy density is estimated by using the results from the previous range to be ?28/9 ≈ ?3.11 against its empirical value of ?3.1. The numerical coefficients in the suggested shapes of the spectrum can be determined by comparison with observational data. Thus, the CR energy spectrumis the result of the random walks of ultrarelativistic particles in energy/momentum space caused by the Fermi mechanism.     

如何编制和预审气象辐射记录月报表

根据编制和预审气象的实践,结合台站经验,就如何编制好辐射月报表谈谈自己的做法。     

FY-4A AGRI陆地气溶胶光学厚度反演

风云四号A星（FY-4A）是中国第二代静止气象卫星的首颗星,多通道扫描成像辐射计AGRI (Advanced Geosynchronous Radiation Imager)是搭载在FY-4A上的主要光学载荷之一。AGRI具有高频率观测特点（每天观测205次）,在大气气溶胶的遥感高频监测方面具有良好应用潜力,但目前官方还未发布相应的气溶胶数据集。本文旨在针对AGRI数据的特点开发基于地表反射率比值库的反演算法以生产高精度的AGRI气溶胶数据集。本文首先基于再分析数据对去云后的AGRI L1级数据进行气体吸收订正;然后利用背景气溶胶光学厚度AOD(Aerosol Optical Depth)对一个月内的“次暗像元”进行大气校正以获取AGRI 0.65μm和0.83μm通道的地表反射率,进而获取这两个通道的地表反射率的比值,完成每个月的地表反射率比值库的构建;最后便可以基于已构建的地表反射率比值库实现地气解耦,完成气溶胶的遥感反演。该算法已被应用于2019年5—10月京津冀地区的气溶胶反演,AGRI AOD反演结果与美国国家航天局发布的MODIS (Moderate-resolution ...     

航空物探对华南某地区天然放射性辐射环境的调查

在华南某地区开展了航空物探调查,发现该地区天然放射性辐射水平相当高,并查明了引起的地质因素和分布特征,评估了天然放射性高辐射地区居民平均有效接收剂量,讨论了人类活动导致富含放射性石料的搬运、扩散所致使的危害.航空物探资料的利用为环境保护和治理规划提供了重要依据.     

海雾生成过程中平流、湍流、辐射效应研究

推导出一个相对湿度方程,分析了在海雾生成过程中平流、湍流和辐射的效应.