简介:Therehavebeen12possiblelocationsoftheearthquakesoccurringintheSouthYellowSeasince1505.Inthispaper,thelocationoftheearthquakethatoccurredin1505hasbeendeterminedbythecollectionofmorehistoricaldataoftheinfluencedfield,referringtheisoseismaldataofearthquakeswiththeepicentralintensityⅨandcombininggeophysicalfielddatawithtectoniccondition,duetoitsgreatinfluenceonseismicsafetyassessmentofsomesignificantengineering.
简介:Anovelautomaticseamlessstitchingmethodispresented.Comparedtothetraditionalmethod,itcanspeedtheprocessingandminimizetheutilizationofhumanresourcestoproducegloballunarmap.Meanwhile,anewglobalimagemapoftheMoonwithspatialresolutionof~120mhasbeencompletedbytheproposedmethodfromChang’E-1CCDimagedata.
简介:以地星状星云(PN)是由高度演化的AGB星在一个非常短的时标内(-10^4年)形成的。因此现在认为即是不是全部,许多PN的周围将保留AGB星的中性包层遗迹。分子的观测是示踪PN中性包层的重要控针。1991年10月使用美国五大学射电天文台(FCRAO)的14-m和QUARRY接收系统对两个较年青的行星状星云M1-7和M1-16以及一个年老的行星状星云VV47进行了COJ=1-0的谱线成图观测,得到了这些星云CO谱线积分强度的空间分布和谱线发射的速度范围。主要结果如下:(1)M1-7的CO(1-0)发射类似CO(2-1)的接近于球形分布,整个辐射区略向东北-西南方向倾斜,且稍大于CO(2-1)的发射区,约为44″×44″。,而膨胀速度则小于CO(2-1)的结果,约为20km/s。(2)M1-16是我们观测样本中光学星云最小的一个年青PN(-3″.6)。没有找到对应CO(2-1)成图资料。我们的观测表明,CO(1-0)的分子射区呈椭圆形壳层结构。△α×△δ-82″×45″。可见尽管源的星云半径很小,但分子发射区有很大的促展。该源的CO(1-0)包层的膨胀速度类似M1-7也小于CO(2-1)的,大约是20km/s。边一现象味着COJ=1-0跃迁相对2-1跃迁而言分布在离电离星云较远的部分。(3)VV47是一个年老的行星状星云。最近Bachiller等人用CO(2-1)跃迁对该源进行观测,在-45,-60和-68km/s等3个速度特征上得到了VV47的两个团块型分子凝聚区,它们播散在东南和西北两个区域。我们用QUARRY系统对VV47周围12′.6×15′.0区域进行了长积分时间的CO(1-0)成图测量,共得到了4个谱特征;在VV47的西北区域有-60和-70km/s两个特征,在东南区域有-45和-34.5km/s两个特征。这最后一个特征暗在CO(2-1)观测中没有发现的。由不同特征速度附近CO(1-0)的谱线积分强度空间分布图可见,对于�
简介:AnearthquakewithM7.1occurredinYushu,QinghaiProvince,China,at07:49a.m.onApril14,2010,accordingtotheChineseSeismicStationNetwork.Thesequenceisafore-mainafter-shocktypesequence.AforeshockwithM4.7occurred2hoursand11minutesbeforethemainshock.Therewere12foreshocksand2385aftershocksuntilJune31,2010.Inwhich,thereare21aftershocksbetweenM3.0andM3.
简介:用被动微波辐射计的陆地检索对在陆地亮度温度的小变化敏感。因此,无线电频率干扰(射频干扰)发信号发出从人造微波放射传输器能在陆地检索导致大错误。在隧道能遥远地污染的C乐队和X乐队的射频干扰察觉到大小,经历了与扫描辐射计(AMSR-E)和WindSat传感器的先进微波。在这个工作,射频干扰察觉的应用程序和在从AMSR-E大小使用检索地球物理的参数的一间全面套房的修正算法,一个维的变化检索(1-DVAR)方法被描述。结果显示检索参数的值例如陆地皮肤温度(LST),在射频干扰污染的这些区域上比从全球数据吸收系统(GDAS)的那些高得多产品。结果也显示新检索和GDAS产品之间的差别通过考虑RFI修正算法显然被减少。另外,1-DVAR的集中度量标准(2)被发现是为识别陆地检索被射频干扰影响的区域的一个新方法。例如在有强壮得多的射频干扰的那些区域,例如欧洲和日本,<啜class=“a-plus-plus”>1-DVAR的2那么大集中不能被到达,检索结果不能是可靠的或不能被获得。而且,<啜class=“a-plus-plus”>2也与中等或弱的射频干扰为那些区域与改正射频干扰的算法减少。射频干扰的结果检测了由<啜class=“a-plus-plus”>2与那些识别了由几乎一致光谱差别方法。
简介:TheElNino-SouthernOscillation(ENSO)ismodulatedbymanyfactors;mostpreviousstudieshaveemphasizedtherolesofwindstressandheatfluxinthetropicalPacific.Freshwaterflux(FWF)isanotherenvironmentalforcingtotheocean;itseffectandtherelatedoceansalinityvariabilityintheENSOregionhavebeenofincreasedinterestrecently.Currently,accuratequantificationsoftheFWFrolesintheclimateremainchallenging;therelatedobservationsandcoupledocean-atmospheremodelinginvolvelargeelementsofuncertainty.Inthisstudy,weutilizedsatellite-baseddatatorepresentFWF-inducedfeedbackinthetropicalPacificclimatesystem;wethenincorporatedthesedataintoahybridcoupledocean-atmospheremodel(HCM)toquantifyitseffectsonENSO.AnewmechanismwasrevealedbywhichinterannualFWFforcingmodulatesENSOinasignificantway.Asadirectforcing,FWFexertsasignificantinfluenceontheoceanthroughseasurfacesalinity(SSS)andbuoyancyflux(QB)inthewestern-centraltropicalPacific.TheSSSperturbationsdirectlyinducedbyENSO-relatedinterannualFWFvariabilityaffectthestabilityandmixingintheupperocean.Atthesametime,theENSO-inducedFWFhasacompensatingeffectonheatflux,actingtoreduceinterannualQBvariabilityduringENSOcycles.TheseFWF-inducedprocessesintheoceantendtomodulatetheverticalmixingandentrainmentintheupperocean,enhancingcoolingduringLaNinaandenhancingwarmingduringElNino,respectively.TheinterannualFWFforcing-inducedpositivefeedbackactstoenhanceENSOamplitudeandlengthenitstimescalesinthetropicalPacificcoupledclimatesystem.
简介:InordertoexploretheabnormalvariationsbeforeandaftertheWen'anM5.1earthquakeonJuly4,2006,thegravitydataobservedbytheWenbaGravityObservationNetworkbeforeandaftertheearthquakewasanalyzed.Therelationshipsbetweengravitychangeandverticaldisplacementandshallowgroundwaterlevelwerediscussed,andelevationcorrectionofthegravitywaspreliminarilyperformed.TheresultsshowthattherewereabnormalgravitychangesbeforetheM5.1earthquake,whichappearedasgravityrisinginthewholeobservationnetwork,especiallyinthesouthpart.AhighgradientofgravityvariationappearedaroundtheepicenterbeforetheM5.1earthquake,especiallyduringtheshortperiodbetweenOctober2005toApril2006.TheboundaryofthepositiveandnegativegravityvariationsgraduallydeflectedandbegantorecoverfromOctober2007.
简介:ApplicationofcertaintyfactorsofearthquakeprecursoryanomalyevidencesCF(E)ZHAO-BIZHENG(郑兆),JUNZHANG(张军)andMEIQING(庆梅)Seismolo...
简介:一、地震基本参数表1 地震基本参数表发震时间年月日时分秒震 中 位 置微 观宏 观东经北纬东经北纬参考地名震级(MS)震源深度(Km)震中烈度 地震类型 196804011705051181°247°117°32′24°54′华安新圩52Ⅵ+主余震型 宏观震中是取Ⅵ度等震线的中心位置,位于华安县新圩南,与微观震中有较大偏离,微观震中在同安县城西南,两者之间相距约60公里。二、地震烈度分布本次地震发生于我省地震队伍成立之前的1968年,现场调查工作在三年之后才补充进行。由于极震区的烈度达Ⅵ度强,民房遭受一定程度的损坏,故震中及Ⅵ、Ⅴ度等震级的确定是可信的,但Ⅳ度线就无从勾划了。图1-1为本次地
简介:Amapoftheaverageatomicnumberoflunarrockandsoilcanbeusedtodifferentiatelithologyandsoiltypeonthelunarsurface.Thispaperestablishesalinearrelationshipbetweentheaverageatomicnumberoflunarrockorsoilandthefluxofpositionannihilationradiation(0.512-MeVgamma-ray)fromthelunarsurface.TherelationshipisconfirmedbyMonteCarlosimulationwithdatafromlunarrockorsoilsamplescollectedbyLuna(Russia)andApollo(USA)missions.AmapoftheaverageatomicnumberofthelunarrockandsoilonthelunarsurfacehasbeenderivedfromtheGamma-RaySpectrometerdatacollectedbyChang’e-1,anunmannedChineselunar-orbitingspacecraft.Inthemap,thehigheraverageatomicnumbers(ZA>12.5),whicharerelatedtodifferenttypesofbasalt,areinthemariaregion;thehighestZA(13.2)readingsareassociatedwithSinusAestuum.ThemiddleZA(~12.1)regions,intheshapeofirregularovalrings,areinWestOceanusProcellarumandMareFrigoris,whichseemstobeconsistentwiththedistributionofpotassium,rareearthelements,andphosphorusasauniquefeatureonthelunarsurface.Theloweraverageatomicnumbers(ZA<11.5)arefoundtobecorrelatedwiththeanorthositeonthefarsideoftheMoon.