倾听地球的诉说—关于地震相互作用的述评     

罗夫  LJ 李丽 《地震科技情报》1993,(12):28-29

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H2 in interstellar and extragalactic ices: infrared characteristics, ultraviolet production, and implications     

Sandford SA  Allamandola LJ 《The Astrophysical journal》1993,409(2):L65-L68

H2 is the most abundant molecule in the universe. We demonstrate that this molecule may be an important component of interstellar and possibly intergalactic ices, both because it can be formed in situ, within the ices, and because gas phase H2 can freeze out onto dust grains in some astrophysical environments. The condensation-sublimation and infrared spectral properties of ices containing H2 are presented. We show that solid H2 in H20-rich ices can be detected by an infrared absorption band at 4137 cm-1 (2.417 micrometers). The surface binding energy of H2 to H2O ice was measured to the delta Hs/k = 555 +/- 35 K. Surface binding energies can be used to calculate the residence times of H2 on grain surfaces as a function of temperature. Some of the implications of these results are considered.  相似文献   

The condensation and vaporization behavior of ices containing SO2, H2S, and CO2: implications for Io     

Sandford SA  Allamandola LJ 《Icarus》1993,106(2):478-488

In an extension of previously reported work on ices containing CO, CO2, H2O, CH3OH, NH3, and H2, measurements of the physical and infrared spectral properties of ices containing molecules relevant to Jupiter's moon Io are presented. These include studies on ice systems containing SO2, H2S, and CO2. The condensation and sublimation behaviors of each ice system and surface binding energies of their components are discussed. The surface binding energies can be used to calculate the residence times of the molecules on a surface as a function of temperature and thus represent important parameters for any calculation that attempts to model the transport of these molecules on Io's surface. The derived values indicate that SO2 frosts on Io are likely to anneal rapidly, resulting in less fluffy, "glassy" ices and that H2S can be trapped in the SO2 ices of Io during night-time hours provided that SO2 deposition rates are on the order of 5 micrometers/hr or larger.  相似文献   

“全面禁止核试验条约”的数据宝藏     

R．Stone朱大庆  吕春来许绍燮 《世界地震译丛》2003,(3):59-62

一个旨在检测核爆炸的传感器台网可以帮助科学家研究从鲸鱼到火山的一切事情。但它们被允许使用吗?  相似文献   

地震学中的统计学原理（二）     

D．Vere-Jones Y．Ogata何阳波  王丽凤邢自兴  刘文兵马丽陈学忠  吕春来 《世界地震译丛》2003,(6):72-82

3.4 模型检验模型检验即检查选用模型的特征与实际样本特征是否一致。选择模型与检验模型采用不相交的数据集较为理想。在做不到这一点的地方,检验需要考虑到模型已被调整到尽可能与数据密切拟合的事实,至少在某种意义上如此。  相似文献   

地下水资源的可持续性长期合理管理     

布朗.  LJ  韩如 《国土资源信息化》1997,(4):16-20

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大陆地壳（二）     

W．D．Mooney 郑文俊楼海  吕春来 《世界地震译丛》2004,(2):79-84

全球地壳厚度等值线图(图6)显示了地壳厚度的双峰标度。海洋盆地的地壳厚度为6～7km(不包括4～5km的水层)，而大陆部分的平均厚度为39．7km。在海洋一大陆边缘的典型地壳厚度是30km，并向大陆内部逐渐增厚到40～45km。厚度超过50km的地壳局限在几个地区，包括中国西部的青  相似文献   

海底地震观测系统     

T.Kanazawa H.Shiobara M.Mochizuki M.Shinohara E.Araki周公威  郝春月吕春来 《世界地震译丛》2004,(5):86-88

基于OHP计划研制了几种类型的海底地震观测系统。本文将介绍这些观测系统，研制的关键是使这个宽频带系统能够长期使用，并且轻便、稳定和耐用。  相似文献   

苏门答腊地震引发毁灭性海啸     

R．Showstack吕春来  陈运泰 《世界地震译丛》2004,(6):79-79

据美国国家海洋与大气管理局太平洋海底环境实验室主任E．Bernard说，印度尼西亚苏门答腊北部以西近海12月26日M9．0级地震随后的毁灭性海啸“据我们所知是第一次全球性的海啸。”  相似文献   

由ODP Leg191布设的海底井下宽频带地震仪系统     

M．Shinohara  E．Araki  T．Kanazawa  M．Mochizuki  K．Hirata  K．Suyehiro  H．Mikada  T．Yamada  Y．Kaiho  周公威  郝春月  吕春来 《世界地震译丛》2004,(6):80-82

名为WP-2的新井下地震观测站由ODP Leg191成功地布设在西北太平洋海盆的ODP1179E钻孔。为了研究地球构造，WP-2台站被安置在一个独特的点位。两套宽频带地震仪用水泥固定在玄武岩层内，通过ROV号潜艇来驱动系统并检查系统的工作状态。ROV也用于回收初始数据。WP-2台站的地震噪声水平对地震观测而言是足够低的。  相似文献