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71.
72.
E. Mahieu C. P. Rinsland R. Zander P. Demoulin L. Delbouille G. Roland 《Journal of Atmospheric Chemistry》1995,20(3):299-310
A set of high-resolution IR solar spectra recorded at the International Scientific Station of the Jungfraujoch, Switzerland, from 84/06 to 93/06, and at the National Solar Observatory McMath-Pierce solar telescope facility on Kitt Peak, Arizona, U.S.A. from 78/05 to 92/07 have been analyzed to determine the vertical column abundances of hydrogen cyanide, HCN, above the two stations. The analysis was based on least-squares curve fitting of calculated spectra to the observations encompassing the P4 and the P8 lines of HCN respectively located at 3299.5273 and 3287.2483 cm–1. The results obtained for the two stations indicate that no significant long-term trend affects either of the two databases; however, this analysis reveals variable increases during springtime of up to a factor of 2 in the HCN total column above the Jungfraujoch and even up to 3 above Kitt Peak. The calculated mean vertical column abundances, excluding the spring observations, are equal to (2.55±0.30)×1015 molec./cm2 (S.D.) and (2.75±0.30)×1015 molec./cm2 respectively above the Jungfraujoch and the Kitt Peak observatories. Based on a realistic volume mixing ratio profile, these columns translate into mean volume mixing ratios equal to 190×10–12 ppv at the respective altitudes of the stations. 相似文献
73.
The ultraviolet absorption cross sections were measured for CF3Br, CF2ClBr, CF2Br-CF2Br, CF2Br2, CHF2Br, CHFBr-CF3, CH2Br-CF3, CHClBr-CF3 in the wavelength range 190–320 nm at 295 K. The photolysis is concluded to be the minor atmospheric sink for CHF2Br, CHFBr-CF3, CH2Br-CF3, CHClBr-CF3. 相似文献
74.
景元书 《南京气象学院学报》1995,18(2):207-212
以试验区实测资料为基础,根据泡桐的树形特征和太阳辐射在树冠中的传播特性,建立了晴、昙、阴不同天气条件下各种密度农桐间作田内太阳辐射的分布模式,较好地体现了间作地辐射日变化趋势。并分析了影响辐射分布的因素,为配置合理的间作模式提供依据。 相似文献
75.
本文通过比较太阳直射表和太阳光度计探测的大气柱气溶胶光学厚度,分析了从太阳直射表探测的全波段太阳直射光强信息确定大气柱气溶胶光学厚度的误差,并应用北京观象台的太阳直射表观测资料,反演得到了 1990—1993年北京大气柱气溶胶光学厚度,分析了该光学厚度月与年变化规律以及1991年菲律宾皮纳图博火山爆发对北京大气气溶胶含量的影响。本文还提出了关于有效水汽含量的一个经验关系式,用于确定水汽对太阳辐射的吸收率。 相似文献
76.
77.
牛广林 《吉林大学学报(地球科学版)》1987,(3)
本文以太阳系星球的物质状态、形态面貌、体积、物质密度、运动速度、运动方向和角动量等作为根据,研究它们在宇宙空间上的分布特点、相互关系、内在联系以及规律的基础上,提出太阳系(乃至宇宙星球)是在46亿年前,宇宙中一个巨大灼热的星球,在高速度左旋旋转(公转和自转)运动的过程中,从尾部分离出来的物质,经过……恒星、行星和卫星依次波状旋转分离运动产生的。 相似文献
78.
Electromagnetic radiation, in its passage through the atmosphere, is attenuated by absorption and scattering by atmospheric
gases, dust and aerosols. The most important absorber is water vapour and the most significant parameter in atmospheric absorption
studies is the total precipitable water in the atmosphere. The present paper summarises the results of a study made to compute
the total precipitable water in the atmosphere over India using radiosonde and other data, as part of a programme for the
computation of direct, global and diffuse solar radiation at the ground from the solar constant. Using values of air temperature
and dew point from the ground up to 250 mb at 19 radiosonde stations and surface water vapour mixing ratio values at 105 surface
observatories in India, precipitable water amounts have been computed for 124 stations, for each month and for the whole year.
The paper describes the techniques used to extend the total precipitable water amounts derived from radiosonde data at 19
stations to 124 stations covering the major climatic zones in the country and presents the results in the form of 12 maps
showing the spatial and temporal distribution of total precipitable water over India 相似文献
79.
Jacques M. Beckers 《Experimental Astronomy》2001,12(1):1-20
In this article I describe a site survey facility, which measures the signals of the solar equivalent of a Differential Image Motion Monitor (S-DIMM) and of a six element linear array of solar scintillometers. Combining the S-DIMM r
o andscintillometer I observations allows the determination of the fractions of the seeing in the free atmosphere and in the ground/lake layer. From the scintillometer array observations C
n
2
(h) is determined for heights corresponding to the first 500 m along the line-of-sight. With minor changes this seeing monitor can also be used for other extended objects like the Moon and planets. 相似文献
80.
E.V. Pitjeva 《Celestial Mechanics and Dynamical Astronomy》2001,80(3-4):249-271
The JPL planetary and lunar ephemerides – DE200/LE200, DE403/LE403, DE405/LE405 and the planetary and lunar ephemerides, EPM87, EPM98, and EPM2000, constructed in the Institute of Applied Astronomy of RAS are described. Common properties and differences of the various ephemerides are given. Graphical comparisons of the DE ephemerides with each other and with the EPM ephemerides are presented. A fairly good agreement of planetary orbits is between DE403, DE405 and EPM98, EPM2000, respectively, over the interval of 120 years (1886–2006) covered by EPM98 and EPM2000. Some differences are explained by a slight disagreement in representing the orbits of Ceres, Pallas, and Vesta as they affect the planets. The accurate radar observations of planets and spacecraft make it possible not only to improve the orbital elements of planets but to determine a broad set of astronomical constants as well: km/AU, parameters of Mars rotation including its precessional rate, the masses of Jupiter, Ceres, Pallas, and Vesta, relativistic parameters of the PPN formalism, the variability of the gravitational constant G. These have been obtained in the fitting process of the DE405 and EPM2000 ephemerides to observational data, including nearly 80000 American and Russian radar observations of planets (1961–1997), ranging and doppler to the Viking and Pathfinder landers, and other miscellaneous measurements from various sources and spacecraft. 相似文献