探空气球施放筒设计     

文永仁  赵毅勇  陈士英  王继凤  祝景先  戴玉芝 《气象科技》2013,41(4):635-638

探空气球的充灌和施放是高空气象观测工作的重要组成部分.目前高空观测中雷达跟踪探空仪、探空信号接收和数据处理都已经实现自动化,只有探空气球的充灌和施放是人工操作,气球充灌氢气有一定危险性,且至少需要一个观测员来完成施放气球工作.该文在分析探空气球充灌和施放各环节工作的基础上,介绍了一种探空气球施放筒的设计方案,以及在业务试验中存在的问题和改进方法,为高空气象观测系统的全程自动化创造条件.  相似文献   

温室黄瓜低温气象灾害指标   总被引：4，自引：0，他引：4  

彭晓丹  杨再强  柳笛  张婷华  周志龙  朱凯  赵翔 《气象科技》2013,41(2):394-400

以黄瓜品种津优35号(Jingyou 35)为试材,于2011年设计不同低温（5、7、9、11 ℃,以25 ℃为对照）处理的人工环境控制试验,系统研究不同低温胁迫对黄瓜叶片光合作用特性及抗氧化酶活性的影响。结果表明：黄瓜叶片最大光合速率随低温胁迫程度的增加依次降低;在不同低温胁迫下,随胁迫时间的延长,黄瓜叶片光补偿点不断升高,光饱和点不断降低;在5 ℃、7 ℃和9 ℃低温处理下,随胁迫时间的延长,光系统Ⅱ最大光化学效率呈下降趋势,光化学淬灭不断降低,非光化学淬灭的变化趋势相反;黄瓜叶片中的超氧化物歧化酶活性随着处理温度的降低先升高后下降;过氧化物酶活性在9 ℃处理24 h后达到最高;过氧化氢酶活性随着处理温度的降低而升高;丙二醛含量大于对照,随胁迫程度的增加先升高,后略有下降。通过研究建立了温室黄瓜低温气象灾害指标,划分为4个等级,分别为轻度、中度、重度和极重,可为设施农业气象服务提供科学依据。  相似文献   

The amino acid composition of the Sutter's Mill CM2 carbonaceous chondrite     

Aaron S. Burton  Daniel P. Glavin  Jamie E. Elsila  Jason P. Dworkin  Peter Jenniskens  Qing‐Zhu Yin 《Meteoritics & planetary science》2014,49(11):2074-2086

We determined the abundances and enantiomeric compositions of amino acids in Sutter's Mill fragment #2 (designated SM2) recovered prior to heavy rains that fell April 25–26, 2012, and two other meteorite fragments, SM12 and SM51, that were recovered postrain. We also determined the abundance, enantiomeric, and isotopic compositions of amino acids in soil from the recovery site of fragment SM51. The three meteorite stones experienced terrestrial amino acid contamination, as evidenced by the low d/l ratios of several proteinogenic amino acids. The d/l ratios were higher in SM2 than in SM12 and SM51, consistent with rain introducing additional l‐ amino acid contaminants to SM12 and SM51. Higher percentages of glycine, β‐alanine, and γ‐amino‐n‐butyric acid were observed in free form in SM2 and SM51 compared with the soil, suggesting that these free amino acids may be indigenous. Trace levels of d +l‐ β‐aminoisobutyric acid (β‐AIB) observed in all three meteorites are not easily explained as terrestrial contamination, as β‐AIB is rare on Earth and was not detected in the soil. Bulk carbon and nitrogen and isotopic ratios of the SM samples and the soil also indicate terrestrial contamination, as does compound‐specific isotopic analysis of the amino acids in the soil. The amino acid abundances in SM2, the most pristine SM meteorite analyzed here, are approximately 20‐fold lower than in the Murchison CM2 carbonaceous chondrite. This may be due to thermal metamorphism in the Sutter's Mill parent body at temperatures greater than observed for other aqueously altered CM2 meteorites.  相似文献   

Presolar grains in the CM2 chondrite Sutter's Mill     

Xuchao Zhao  Yangting Lin  Qing‐Zhu Yin  Jianchao Zhang  Jialong Hao  Michael Zolensky  Peter Jenniskens 《Meteoritics & planetary science》2014,49(11):2038-2046

The Sutter's Mill (SM) carbonaceous chondrite is a regolith breccia, composed predominantly of CM2 clasts with varying degrees of aqueous alteration and thermal metamorphism. An investigation of presolar grains in four Sutter's Mill sections, SM43, SM51, SM2‐4, and SM18, was carried out using NanoSIMS ion mapping technique. A total of 37 C‐anomalous grains and one O‐anomalous grain have been identified, indicating an abundance of 63 ppm for presolar C‐anomalous grains and 2 ppm for presolar oxides. Thirty‐one silicon carbide (SiC), five carbonaceous grains, and one Al‐oxide (Al₂O₃) were confirmed based on their elemental compositions determined by C‐N‐Si and O‐Si‐Mg‐Al isotopic measurements. The overall abundance of SiC grains in Sutter's Mill (55 ppm) is consistent with those in other CM chondrites. The absence of presolar silicates in Sutter's Mill suggests that they were destroyed by aqueous alteration on the parent asteroid. Furthermore, SM2‐4 shows heterogeneous distributions of presolar SiC grains (12–54 ppm) in different matrix areas, indicating that the fine‐grained matrix clasts come from different sources, with various thermal histories, in the solar nebula.  相似文献   

Records of the Moon‐forming impact and the 470 Ma disruption of the L chondrite parent body in the asteroid belt from U‐Pb apatite ages of Novato (L6)     

Qing‐Zhu Yin  Qin Zhou  Qiu‐Li Li  Xian‐Hua Li  Yu Liu  Guo‐Qiang Tang  Alexander N. Krot  Peter Jenniskens 《Meteoritics & planetary science》2014,49(8):1426-1439

Novato, a newly observed fall in the San Francisco Bay area, is a shocked and brecciated L6 ordinary chondrite containing dark and light lithologies. We have investigated the U‐Pb isotope systematics of coarse Cl‐apatite grains of metamorphic origin in Novato with a large geometry ion microprobe. The U‐Pb systematics of Novato apatite reveals an upper intercept age of 4472 ± 31 Ma and lower intercept age of 473 ± 38 Ma. The upper intercept age is within error identical to the U‐Pb apatite age of 4452 ± 21 Ma measured in the Chelyabinsk LL5 chondrite. This age is interpreted to reflect a massive collisional resetting event due to a large impact associated with the peak arrival time at the primordial asteroid belt of ejecta debris from the Moon‐forming giant impact on Earth. The lower intercept age is consistent with the most precisely dated Ar‐Ar ages of 470 ± 6 Ma of shocked L chondrites, and the fossil meteorites and extraterrestrial chromite relicts found in Ordovician limestones with an age of 467.3 ± 1.6 Ma in Sweden and China. The lower intercept age reflects a major disturbance related to the catastrophic disruption of the L chondrite parent body most likely associated with the Gefion asteroid family, which produced an initially intense meteorite bombardment of the Earth in Ordovician period and reset and degassed at least approximately 35% of the L chondrite falls today. We predict that the 470 Ma impact event is likely to be found on the Moon and Mars, if not Mercury.  相似文献   

Chromium isotopic systematics of the Sutter's Mill carbonaceous chondrite: Implications for isotopic heterogeneities of the early solar system     

Akane Yamakawa  Qing‐Zhu Yin 《Meteoritics & planetary science》2014,49(11):2118-2127

Recent studies have shown that major meteorite groups possess their own characteristic ⁵⁴Cr values, demonstrating the utility of Cr isotopes for identifying genetic relationships between the planetary materials in conjunction with other classical tools, such as oxygen isotopes. In this study, we performed Cr isotope analyses for whole rocks and chemically separated phases of the new CM2 chondrite, Sutter's Mill (SM 43 and 51). The two whole rocks of Sutter's Mill show essentially identical ε⁵⁴Cr excesses (SM 43 = +0.95 ± 0.09ε, SM 51 = +0.88 ± 0.07ε), relative to the Earth. These values are the same within error with that of the CM2‐type Murchison (+0.89 ± 0.08ε), suggesting that parent bodies of Sutter's Mill and Murchison were formed from the same precursor materials in the solar nebula. Large ε⁵⁴Cr excess of up to 29.40ε is observed in the silicate phase of Sutter's Mill, while that of Murchison shows 15.74ε. Importantly, the leachate fractions of both Sutter's Mill and Murchison form a steep linear anticorrelation between ε⁵⁴Cr and ε⁵³Cr, cross‐cutting the positive correlation previously observed in carbonaceous chondrites. The fact that L4 acid leachate fraction contains higher ⁵⁴Cr excesses than that of L5 step designed to dissolve refractory minerals suggests that spinel is not a major ⁵⁴Cr carrier. We also note that L5 contains ⁵³Cr anomalies lower than the solar initial value, suggesting it carries a component of nucleosynthetic anomaly unrelated to the ⁵³Mn decay. We have identified five endmember components of nucleosynthetic origin among the early solar system materials.  相似文献   

Photometric Studies of Twelve Deep, Low-mass Ratio Overcontact Binary Systems     

Qian Shengbang  Yang Yuangui  Zhu Liying  He Jiajia  Yuan Jingzhao 《Astrophysics and Space Science》2006,304(1-4):25-28

The formations of the blue straggler stars and the FK Com-type stars are unsolved problems in stellar astrophysics. One of the possibilities for their formations is from the coalescence of W UMa-type overcontact binary systems. Therefore, deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars are a very important source to understand the phenomena of Blue Straggler/FK Com-type stars. Recently, 12 W UMa-type binary stars, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, V410 Aur, XY Boo, SX CrV, QX And, GSC 619-232, and AH Cnc, were investigated photometrically. Apart from TV Mus, XY boo, and GSC 619-232, new observations of the other 9 binaries were obtained. Complete light curves of the 10 systems, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, GSC 619-232, V410 Aur, XY Boo, and AH Cnc, were analyzed with the 2003 version of the W-D code. It is shown that all of those systems are deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars. We found that the system GSC 619-232 has the highest degree of overcontact (f = 93.4%). The derived photometric mass ratio of V857 Her, q = 0.0653, indicates that it is the lowest-mass ratio system among W UMa-type binaries.Of the 12 sample stars, long-term period changes of 11 systems were found. About 58% (seven) of the sample binaries show cyclic period oscillation. No cyclic period changes were discovered for the other 5 systems, which may be caused by the short observational time interval or by insufficient observations. Therefore, we think that all W UMa-type binary stars may contain cyclic period variations. By considering the long-term period changes (both increase and decrease) of those binary stars, we proposed two evolutionary scenarios evolving from deep, low-mass ratio overcontact binaries into Blue Straggler/FK Com-type stars.  相似文献   

用GPS位移资料计算应变方法的讨论   总被引：48，自引：20，他引：28  

石耀霖  朱守彪 《大地测量与地球动力学》2006,26(1):1-8

目前使用相同或类似的GPS资料求应变,不同研究者给出的结果会有显著差别。为此,对用GPS位移(或速度)资料计算应变(或应变速率)的方法进行了研讨。分析后认为,应变计算可以归结成两大类第一类是利用测点附近资料直接求微分或微分的加权平均值的直接计算法;第二类是用解析曲线拟合观测的位移,然后根据该曲线提供的总的趋势求测点的微分值的位移拟合法,这类方法在拟合中又可以分成整体拟合和分片拟合两种。应变计算应该在球面坐标系下进行,根据研究对象和要求,选择适当的方法。  相似文献   

科学计算程序库WHIGG F90 LIB及其地学应用   总被引：3，自引：1，他引：2  

闫昊明  钟敏  朱耀仲 《大地测量与地球动力学》2006,26(1):109-114

WHIGG F90LIB(WFL)是一款用FORTRAN90语言编写的用于地球学科的计算程序库。应用WFL可以减少重复性编程,方便地解决科学计算中数据的预处理问题,结合多种分析方法,对科学问题进行定量分析。利用WFL在地球重力场、气候涛动和数字信号处理3个方面的应用实例,以验证WFL在科学计算中应用的有效性。  相似文献   

中国地壳运动观测网络GPS观测方案优化研究   总被引：2，自引：2，他引：0  

王文萍  王庆良  朱桂芝 《大地测量与地球动力学》2002,22(3):60-65

中国地壳运动观测网络GPS区域站采用了严格同步环、连续4天、高站点重复率的观测方案，为了优化观测方案，以青藏块体东北缘GPS区域网1999年和2001年观测资料为例，对区域GPS观测方案进行了对比试验和分析。结果表明：①同步环连续3天和连续4天观测的基线重复率和站点速度结果基本一致，可以采用站点连续3天观测的方案；②异步环有站点重复观测与无站点重复观测对比，站点速度差别很小（亚毫米级），优化观测时可以大大降低或取消异步环站点重复率；③同步环整体解算（带IGS站）与环内站点单独触算（带IGS站），其站点速率差异可达1mm以上，因此优化观测时还应尽量采用同步环观测方案。  相似文献