关于【单亲家庭的男孩子都有哪些心理问题】，单亲家庭男孩心理问题，今天向乾小编给您分享一下，如果对您有所帮助别忘了关注本站哦。
内容导航：1、会议通知｜GNSS电离层国际研讨会（IWGI2018）2、单亲家庭的男孩子都有哪些心理问题：单亲家庭男孩心理问题1、会议通知｜GNSS电离层国际研讨会（IWGI2018）
《测绘学报》
构建与学术的桥梁 拉近与权威的距离
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Background & Objectives
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Ionospheric delay is one of main GNSS errors, which is still challenging to precisely correct and model the ionospheric error in positioning, navigation and timing (PNT). Nowadays, dual-frequency GNSS observations can precisely estimate ionoispheric delay, total electron content (TEC), electron density etc, which provide a unique opportunity to correct, monitor and understand ionospheric variations, particularly multi-GNSS, including US's GPS, Russia's GLONASS, China's BeiDou and EU's Galileo as well as regional systems, such as Japan's QZSS and India's IRNSS.The International Workshop on GNSS Ionosphere (IWGI2018) - Observations, Advances and Opportunities is jointly sponsored by the International Association of Geodesy (IAG), German Aerospace Center (DLR) and Shanghai Astronomical Observatory, CAS, China (SHAO). The IWGI2018 will be held on November 4-6, 2018, Shanghai, China. The IWGI2018 aims to provide a platform for GNSS scientists and engineers to communicate and exchange in GNSS ionosphere theory, methods, technologies, applications and future challenges. The IWGI2018 is open to all scientists who may have the latest results and developments in GNSS ionosphere, including ionospheric delay estimating theory, algorithms, modelling and applications in engineering and Earth/space science as well as combining multi-sensors. Manuscripts on new advances in GNSS ionosphere and space weather are also welcome.
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Sessions & Topics
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Session 1: Multi-GNSS Current Status and Advances
Session 2: GNSS Tropospheric Delay Estimation and Effects
Session 3: GNSS Ionospheric Delay Estimation and Modelling
Session 4: GNSS Ionospheric Tomography and Radio Occultation
Session 5: Ionospheric Delay Effects on Navigation and Positioning
Session 6: Ionospheric/Thermospheric Irregularities from GNSS
Session 7: GNSS Space Weather and Environment Variations
Session 8: Seismic-Ionospheric Disturbances and Warning
Session 9: Ionosphere and Space Environments from Multi-Sensors
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Sponsors
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International Association of Geodesy (IAG)
German Aerospace Center (DLR)
Shanghai Astronomical Observatory (SHAO), China
Nanjing University of Information Science & Technology (NUIST)
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Scientific Organizing Committee (SOC)
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Shuanggen Jin, Shanghai Astronomical Observatory, CAS, China (Chair)
Mainul Hoque, German Aerospace Center (DLR), Germany (Co-Chair)
Sergey Pulinets, Space Research Institute, RAS, Russia
Jens Berdermann, German Aerospace Center (DLR), Germany
Libo Liu, Institute of Geology and Geophysics, CAS, China
Andrzej Krankowski, University of Warmia & Mazury in Olszt, Poland
Charles Lin, National Cheng Kung University, Taiwan
Norbert Jakowski, German Aerospace Center (DLR), Germany
Yunbin Yuan, Institute of Geodesy and Geophysics, CAS, China
Yuichi Otsuka, Ins. Space-Earth Environ., Nagoya University, Japan
Yibin Yao, School of Geodesy & Geomatics, Wuhan Univrsity, China
Manuel Hernandez-Pajares, Universitat Politecnica de Catalunya, Spain
Hong Yuan, Academy of Opto-Electronics (AOE), CAS, China
Michael Schmidt, Technische Universitat Munchen (TUM), Germany
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Local Organizing Committee (LOC)
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Shuanggen Jin, Shanghai Astronomical Observatory, CAS, China (Chair)
Peng Guo, Shanghai Astronomical Observatory, CAS, China
Zhounan Dong, Shanghai Astronomical Observatory, CAS, China
Jiandong Liu, Shanghai Astronomical Observatory, CAS, China
Yang Yu, Shanghai Astronomical Observatory, CAS, China
International Workshop on GNSS Ionosphere (Nov. 5-6, 2018)
Program Handbook
Registration & Payment on-site (Nov. 4-6, 2018)
3rd floor of SHAO Building, Shanghai, China
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Abstract submission
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Please email your abstract with Abstract_IWGI2018_xxx.doc to Mr. Jiandong Liu: ,Registration without abstract
Please email registration form or following information to Mr. Jiandong Liu:First Name :_____________; Last Name: _____________; Title: _____________
Institute :_________________; Country :____________
Address:________________ ; Post code: __________
Email :_______________; Tel: _______________
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Payment Type
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Regular: 250$USD or 1500 RMB
Students: 150$USD or 1000 RMB
Payment by cash
Payment on site by Chinese Yuan, US Dollar or Euro cash
Payment by bank tranfer
Bank transfer (please note usage for IWGI2018). (English version)
Bank transfer (please note usage for IWGI2018). (Chinese version ÖÐÎÄ°æ)
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Participants
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NumberNAMEAFFILIATIONCOUNTRYABSTRACTEMAIL1Libo Liu Institute of Geology and Geophysics, CASChinaIonospheric monitoring and physics: Recent progresses in China liul@mail.iggcas.ac.cn2Norbert Jakowski/M. Mainul Hoque German Aerospace Center (DLR)GermanyFast and improved ionospheric correction by NTCM models using GNSS broadcast coefficientsThe Nighttime Winter Anomaly (NWA) effect - a persistent feature of the mid-latitude ionospheres at the American and Asian longitude sectorsNorbert.Jakowski@dlr.de3Volkan Akgul Bulent Ecevit UniversityTurkeyHigh-order ionopsheric effects on GPS-estimated tropospheric delay gradients akgulvo@gmail.com4Manuel Hernandez-Pajares UPC-IonSAT, Universitat Politecnica de Catalunya SpainPrecise ionospheric electron content monitoring from single-frequency GNSS receivers manuel.hernandez@upc.edu>5Qin Peng Shanghai University & SHAOChinaIonospheric delay effects on significant wave height estimation from CYGNSS GNSS-R observations 79120615@qq.com6Shuanggen Jin Shanghai Astronomical Observatory, CASChinaGNSS cloudy platform for digital space: Advances, applications and opportunities sgjin@shao.ac.cn7Y. Tony Song NASA JPLUSAxxxTony.Song@jpl.nasa.gov8Xiaodong Qian Shanghai Astronomical Observatory, CASChinaIonospheric delay correction for mean sea level change from CYGNSS GNSS-R observations xdqian@shao.ac.cn9Mainul Hoque German Aerospace Center (DLR)GermanyEstimates of higher order ionospheric effects for GNSS signals received onboard LEO satellites Mainul.Hoque@dlr.de10Andres Calabia Shanghai Astronomical Observatory, CASChinaVariations of thermospheric air mass density derived from GRACE accelerations and GPS POD andres@calabia.com11Jiandong Liu Shangha Astronomical Observatory, CASChinaWave distribution and activities in the upper Mars atmosphere from multi-satellite accelerometer observations jd_liu@shao.ac.cn12Jens Berdermann German Aerospace Center (DLR)GermanyxxxJens.Berdermann@dlr.de13Jiuhou Lei University of Science and Technology of ChinaChinaxxxleijh@ustc.edu.cn14Ke Su Shanghai Astronomical Observatory, CASChinaEvaluation of ionospheric ionospheric effects on multi-GNSS PPP performances ksu@shao.ac.cn15Yuichi Otsuka Nagoya UniversityJapanxxxotsuka@isee.nagoya-u.ac.jp16Liangliang Yuan Shanghai Astronomical Observatory, CASChinaThermospheric mass density variations following the September 2017 geomagnetic storm from GRACE and SWARM precise orbits 18905648099@189.cn17Xin Liu Shanghai University & SHAOChinaIonospheric disturbances following the 2011 Tohoku-Oki Tsunami from GPS observations 990528837@qq.com18Chao Gao Shanghai Astronomical Observatory, CASChinaHigh-order ionospheric effects on neutral atmospheric parameters estimation from FY-3C GPS Radio Occultation 349827456@qq.com19Zhonnan Dong Shanghai Astronomical Observatory, CASChina3-D water vapor tomography in Wuhan from GPS, BDS and GLONASS observations zndongcsu@163.com20Charles Lin National Cheng Kung UniversityTaiwan, Chinaxxxcharles@mail.ncku.edu.tw21Ershen Wang Shenyang Aerospace UniversityChinaSatellite Selection Algorithm for Multi-constellation GNSS Positioning wanges_2016@126.com22Yuhan Liu Shanghai University & SHAOChinaIonospheric disturbances following the 2018 Mw=7.9 Alaska earthquake from GPS observations inuyasha471@qq.com23Dasari Prasad Andhra UniversityIndiaLongitudinal variation of GPS TEC and ROTI at equatorial and low latitude IGS stations during declining phase of Solar Cycle 24(presentation) dsvvdprasad@gmail.com24Dasari Prasad Andhra UniversityIndiaVariation of TEC over different longitudes and latitudes of North American sector during the 21st August 2017 total solar eclipse(poster) dsvvdprasad@gmail.com25Virendra Patel Sardar Vallabhbhai National Institute of TechnologyIndiaImpact of ockhi cyclone on IRNSS/NavIC GNSS signal due to ionospheric and tropospheric variation virendra369@gmail.com26Gopal Mondal Jadavpur UniversityIndiaIonospheric variation during El Nino and La Nina years over tropical Pacific Ocean gopalmondal18@gmail.com27Feza Arikan Hacettepe UniversityTurkeyPerformance of IRI-Plas with GIM-TEC input as Compared to Ionosonde Data for Equinox Seasons arikan@hacettepe.edu.tr28Solen Kumbay Yildiz Hacettepe UniversityTurkeyInvestigation of Spatio-Temporal Variability of Midlatitude Ionosphere Using GIM-TEC solen@ee.hacettepe.edu.tr29K.D.Sriniuasu Vadlamurt Andhra UniversityIndiavkdsrinivasu@gmail.com30Yue Deng University of Texas at Arlington USALarge-scale traveling ionospheric disturbances (LSTIDs) and correlation with auroral activity and ion convection pattern: Comparison between GPS-TEC data and GITM simulation yuedeng@uta.edu31Haiyang Fu Fudan University Chinafuhaiyang@gmail.com32Yanhong Chen National space science center,CAS ChinaIonosphere modeling, specification and application from GNSS observation chenyh@nssc.ac.cn33Shun Zhang Shangqiu Normal University ChinaSpatial and temporal patterns of ~27-day oscillation in ionospheric TEC zhangshun@whu.edu.cn>34Wei Geng National Space Science Center, CAS ChinaGeneration of Ionospheric Scintillation Maps over Southern China based on Kriging Method 15201525096@163.com>35Yuxiang Peng Virginia Tech Center for Space Science and Engineering Research USASatellite Formation Flight Simulation Using Multi-constellation GNSS and Applications to Ionospheric Remote Sensing yuxiang7@vt.edu>36Randa Natras Department of Geodesy and Geoinformation, Vienna University of Technology AustriaLocal Ionosphere TEC Model for Bosnia and Herzegovina - Preliminary results randa.natras1@gmail.com>37Randa Natras and Dzana Horozovic Department of Geodesy and Geoinformation, Vienna University of Technology AustriaLatitudinal and Seasonal Dependence of Geomagnetic Storm Effects on the Ionospheric TEC and Positioning Accuracy in Europe in 2015 randa.natras1@gmail.com;dzana.horozovic@geo.tuwien.ac.at>38Liming He Department of Geodesy and Geomatics, Northeastern University ChinaThree-dimensional structure of ionospheric disturbance observed by dense GNSS network heliming@mail.neu.edu.cn>39Zhihuai Guo School of Geodesy and Geomatics, Wuhan University ChinaThe Accuracy Analysis of IRI-2016 and NeQuick2 at Antarctic Area zihuai_Guo@163.com>40Zhou Chen Institute of Space Science and Technology, Nanchang University ChinaImprovement of Deep learning algorithm (DCGAN) for total electron content (TEC) maps yuedeng@uta.edu41Wenfeng Nie Institute of Space Sciences, Shandong University ChinaRevisit the calibration errors on experimental slant total electron content (TEC) determined with GPS wenfengnie@sdu.edu.cn>42Qingtao Wan National Astronomical Observatories of China, Chinese Academy of Sciences ChinaAnalysis of GPS-TEC of the Equatorial Ionization Anomaly around 115oE longitude qtwan@nao.cas.cn>43Dunyong Zheng Hunan University of Science and Technology Chinaxxzdymath@163.com>44Guiwen Lan and Kaiwen Feng College of Geomatics and Geoinformation China3D Visualization of Urban Underground Pipelines with SuperMap and 3DS MAX 290371393@qq.com>45Ningbo Wang Academy of Opto-Electronics,Chinese Academy of Sciences ChinaBDSMART: BDS/GNSS ionospheric Monitoring And Retrieval Terminal for ionosphere sensing wangningbo@aoe.ac.cn>46Ningbo Wang and Zishen Li Academy of Opto-Electronics,Chinese Academy of Sciences ChinaBenefits of IGS RTS for real time ionospheric space weather monitoring wangningbo@aoe.ac.cn>47Wei Shang SHAO,Chinese Academy of Sciences ChinaXX907912215@qq.com>48Xiaolan Wang National Astronomical Observatories of China, Chinese Academy of Sciences ChinaComparison of global ionospheric GPS-TEC measurements with IRI-TEC xlwang@nao.cas.cn>49Chendong Li Department of Civil Engineering, the University of Nottingham ChinaFurther Statistical Analysis of the Correlation between Scintillation Parameters and MP&ROTI Chendong.LI@nottingham.edu.cn>50Chengli She Institute of Geology and Geophysics, Chinese Academy of Sciences ChinaGNSS Ionospheric Delay Estimation from an Individual Multi-GNSS Station certainly@mail.iggcas.ac.cn>51Haixia Lyu GNSS Research Center, Wuhan University; UPC GNSS Research Center, Universitat Politecnica de Catalunya;China/Spainxxhaixia.lyu@upc.edu>52Michael Jehle u-blox AG SwitzerlandXXMichael.Jehle@u-blox.com53Yangyi Sun China University of Geosciences (Wuhan) ChinaEl Nino - Southern Oscillation signature in ionosphere observed by FORMOSAT-3/COSMIC radio occultation sunyy@cug.edu.cn54Kunpeng Shi College of Geodesy and Geomatics, Shandong University of Science and Technology ChinaTemporal-spatial variations of plasma electron content in high and low solar activity year 514026949@qq.com55Jun Chen School of Geodesy and Geomatics, Wuhan University ChinaModeling and analysis of a new ionospheric mapping function cj_snake@whu.edu.cn56Hongda Miao Xidian University ChinaA GPU Model of the Ionosphere Based on Sami2 1925059579@qq.com57Hongda Miao Xidian University ChinaA GPU Model of the Ionosphere Based on Sami2 1925059579@qq.com58XiangXiang Yan Hubei Subsurface Multi-scale Imaging Key Laboratory, China University of Geosciences ChinaVertical structure of the earthquake-induced ionospheric perturbations based on FORMOSAT-3/COSMIC data yanxxcug@foxmail.com59Yongxing Zhu Information Engineering University ChinaAccuracy analysis of broadcasting ionospheric parameters for the latest BDS-3 experimental satellites 18049269002@126.com60Weijun Lu National Astronomical Observatories, CAS ChinaA preliminary result of ionospheric TEC derivation from GPS carrier phase observations luweijun14@mails.ucas.ac.cn61Guoqiang Pang University Of Electronic Science And Technology Of China ChinaA new study of ionospheric delay based on dual-frequency BeiDou reference station GuoqiangPang15@163.com62Conglin Zhou Geomatic Center of Guangxi ChinaAnalysis of the application of GNSS technology in seismic research 573014033@qq.com63Jinghua Li National Astronomical Observatories, CAS ChinaEvaluation of the Klobuchar model in TaiWan jhli@nao.cas.cn64Shuaimin Wang Institute of Space Science, Shandong University ChinaEstablishment of weighted mean temperature model in the polar region wsm1949@sina.com65Biao Jin Institute: Space star technology co., LTD ChinaSBAS Ionospheric Spatial Threat Model and the Integrity in China Area 617630427@qq.com66Mingzhe Li Institute of Geology and Geophysics, CAS ChinaCharacterization of the residual ionospheric errors in neutral radio occultation retrievals limingzhe@mail.iggcas.ac.cn67Mingzhe Li Institute of Geology and Geophysics, CAS ChinaCharacterization of the residual ionospheric errors in neutral radio occultation retrievals limingzhe@mail.iggcas.ac.cn68Hang Liu Xi'an University of Science and Technology Chinaxx673290038@qq.com69Xiaohua Xu School of Geodesy and Geomatics, Wuhan University Chinathe Influence of the Spatial and Temporal Collocation Windows on the Comparisons of the Ionospheric Characteristic Parameters Derived from COSMIC Radio Occultation and Digisondes xhxu@sgg.whu.edu.cn70Jinmei Guo University of Electronic Science and Technology Of China ChinaEstimation of Carrier Phase Deviation of Geometric-free Linear Combination of Beidou Tri-Frequency Signals for Ionospheric TEC Modeling jinmeiguo112@163.com71Yue Hong University of Electronic Science and Technology Of China ChinaEvaluate and mitigate the effects of ionospheric interference on the accuracy and integrity of the BeiDou system 2284434734@qq.com72Xinying Zhong Geomatic Center of Guangxi ChinaPERFORMANCE ANALYSIS OF BEIBU GULF OF GUANGXI BEIDOU NAVIGATION GROUND-BASED AUGMENTATION SYSTEM 351942387@qq.com73Yong Wang Shandong University China/CanadaPolar cap structures and dynamics revealed by TEC keograms extracted from TEC maps wangyong180@163.com>74Yong Wang Shandong University ChinaExperimental evidence on the dependence of the standard GPS phase scintillation index on the ionospheric plasma drift around noon sector of the polar ionosphere wangyong180@163.com>75Pornchai Supnithi King Mongkut's Institute of Technology Ladkrabang ThailandRelationship between Spread -F Events and the Rate of Total Electron Content Change Index (ROTI) in Equatorial Region at Thailand Chumphon Station, Thailand pornchai.su@kmitl.ac.th>76Jiaqi Zhao and Chen Zhou School of Electronic Information, Wuhan University ChinaOn the Optimal Height of Ionospheric Shell for Single-Site TEC Estimation chenzhou@whu.edu.cn;zhaojiaqi@whu.edu.cn>77Dedalo Marchetti Istituto Nazionale di Geofisica e Vulcanologia Nanjing University of Information Science and Technology,China/ItalyPossible pre-earthquake ionospheric anomalies detected by Swarm satellites and a preliminary integration with the new CSES Zhangheng 1 satellite data dedalo_marchetti@yahoo.it78Takashi MARUYAMA National Astronomical Observatories, CASNational Institute of Information and Communications TechnologyChina/JapanPrecise estimation of total electron content by double thin-shell model at equatorial and low latitudes using local receiver network tmaru@nict.go.jp79Jinghua Li National Astronomical Observatories, CAS ChinaEvaluation of the Klobuchar model in TaiWan jhli@nao.cas.cn80Ning Wang National Key Laboratory of Electromagnetic Environment, China Research Institute of Radio-wave PropagationChinaObservations of GPS ionospheric scintillation over Guangzhou in China during the 23rd solar cycle wn_22s_cetc@163.com81Jinyun Guo Shandong University of Science and TechnologyChinaxxjinyunguo1@126.com82Shunrong Zhang MIT Haystack ObservatoryUSAThe 2017 Great America Eclipse induced ionospheric bow waves shunrong@mit.edu83Jianfeng Li School of Earth Science and Environmental Engineering, Southwest Jiaotong UniversityChinaCoupling Characteristics analysis for Ionospheric Storm and Geomagnetic Storm jianfengli@my.swjtu.edu.cn84Guanyi Chen Ionosphere Laboratory, School of Electronic Information, Wuhan UniversityChinaA Statistical Analysis of Medium-scale Traveling Ionospheric Disturbances during 2014-2017 by using data from CORS Network in Hong Kong chenguanyi@whu.edu.cn85Chao Xiong GFZ German Research Centre for Geosciences PotsdamGermanyThe GPS signal interruption of Swarm satellites caused by ionospheric plasma irregularities bear@gfz-potsdam.de86Shunzu Gao Electronic Information School, Wuhan UniversityChinaIntegrated Algorithm for TEC Measurement with GPS and BDS Receivers gaoshz@whu.edu.cn87Kaixuan Zhang University Of Electronic Science And Technology Of China ChinaAccurate ionospheric delay model for real time BDS base positioning of LEO satellites using horizontal VTEC gradient estimatio shaoqiankai@foxmail.com88Yufei Wu University Of Electronic Science And Technology Of China ChinaIonospheric Disturbance Monitoring Based on Convolution Neural Networks 120020435@qq.com89zhengxie Zhang University Of Electronic Science And Technology Of China ChinaReal-Time Extracting Ionospheric Delays and Establishing Regional Model by CORS 15651975330@163.com90Guangyuan Tan National Space Science Center, Chinese Academy of Sciences ChinaError Analysis on NmF2 and HmF2 Parameter of IRI-2016 Model during Magnetically Quiet and Storm Periods tgy8080@126.com91Weihua Bai National Space Science Center, Chinese Academy of Sciences ChinaThe validation and application of ionospheric radio occultation products derived from FY3C/GNOS bjbwh@163.com92Guozhu Li Institute of Geology and Geophysics, Chinese Academy of Sciences ChinaAn introduction to the ionospheric observation network for irregularity and scintillation in East/Southeast Asia (IONISE) gzlee@mail.iggcas.ac.cn93Jieqing Yu School of Environment Science and Spatial Inofrmatics,China University of Mining & Technology ChinaIonospheric tomography by image reconstruction based on hybrid grids yujieqing@cumt.edu.cn94Wenxiang Li Research Institute of Electronic Science and Technology, UESTC ChinaReview of Ionospheric TEC and NmF2 Perturbations Before Wenchuan Earthquake LWX_UESTC@163.com95Shenwei Shi Nanjing University of Information Science & Technology Chinaxxt1142430226@163.com96Jiabing Guo Nanjing University of Information Science & Technology Chinaxx1292196066@qq.com97Yiduo Wen Nanjing University of Information Science & Technology Chinaxx1505006362@qq.com98Naifeng Fu Shanghai Astronomical Observatory, CAS Chinaxxnffu@shao.ac.cn99Peng Guo Shanghai Astronomical Observatory, CASChinaxxxgp@shao.ac.cn100Mengjie Wu Shanghai Astronomical Observatory, CASChinaxxxmjwu@shao.ac.cn101Sergey Pulinets Space Research Institute, RASRussiaxxxpulse1549@gmail.com102Hui Qiu Shanghai Astronomical Observatory, CASChinaxxxws2834825886@163.com103Michael Schmidt Technische Universitat Munchen (TUM)Germanyxxxmg.schmidt@tum.de104Zhaoyang Hong ShanghaiTech University & SHAOChinaxxx504218720@qq.com105Jie Chen Xiangtan University & SHAOChinaxxx422061442@qq.com106Andrzej Krankowski University of Warmia & Mazury in OlsztPolandxxxkand@uwm.edu.pl107Qiang Chen Xiangtan University & SHAOChinaxxx422061442@qq.com108Wei Shang Shanghai University & SHAOChinaxxx90791215@qq.com109Zengji Zheng Shanghai Astronomical Observatory, CASChinaxxx13488316276@126.com110Bahruz Ahadov Shanghai Astronomical Observatory, CASChinaxxxgeofizik608@mail.ru111Shuhua Ye Shanghai Astronomical Observatory, CASChinaxxxysh@shao.ac.cn112Yang Yu Shanghai Astronomical Observatory, CASChinaxxxyuyang@shao.ac.cn113Qinyun Zhang Shanghai University & SHAOChinaxxx915424294@qq.com114Oufang Luo Shanghai Astronomical Observatory, CASChinaxxxofluo@hotmail.com115Xiaojuan Tian Shanghai Astronomical Observatory, CASChinaxxxxjtian@shao.ac.cn116Xuerui Wu Shanghai Astronomical Observatory, CASChinaxxxxrwu@shao.ac.cn117Mostafa S. Abd-Elbaky Shanghai Astronomical Observatory, CASChinaxxxmstabdelbaky@gmail.com118Sheng Liu XAO/SHAO, CASChinaxxxliusheng17@mails.ucas.ac.cn119Hugo Carreno-Luengo Centre Tecnologic de Telecomunicacions de Catalunya (CTTC)Spainxxxhugo.carreno.luengo@gmail.com120Chun Li Xiangtan University & SHAOChinaxxx422061442@qq.com121Yang He Shanghai University & SHAOChinaxxx1137353689@qq.com122Hong Lu Institute of High Energy Physics,CASChinaxxluh@ihep.ac.cn123Ming Ou China Research Institute of Radiowave PropagationChinaxxohm1122@163.com124Jian Feng China Research Institute of Radiowave PropagationChinaxxfengjian428@163.com◆◆
Registration & abstract submission deadline
September 15, 2018 (Extended)Invitation Letter for Visa deadline
September 15, 2018
Pay registration fee deadline (bank transfer)
October 20, 2018
Hotel reservation
October 31, 2018
Notification of acceptance & preliminary programme
September 30, 2018
Registration & Payment on site by Chinese Yuan, US Dollar or Euro cash
November 4, 2018
Conference time
November 5-6, 2018
Social Program
Travelling in Shanghai
Shanghai City
Travelling in China
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inviation&visa
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IWGI2018 Annoucement
Announcement
Invitation Letter
Invitation Letter
Invitation for Visa
One easy way is to apply for Tourist Visa without Invitation Letter for most countries
The other needs more detailed personal information to apply for the official authorized Invitation Letter, please send the following information to Jiandong Liu (jd_liu@shao.ac.cn) (Tel: 86-21-34775291) by September 15, 2018.
Passport copy
Full name as in passport :________________
Passport Number :_____________
Nationality :_______________
Date of Birth :_______________
Position Title :_________________(Post-Doc, Prof. or Head/Director)
Detailed Itinerary From ____ (MM) _____(DD) _______(YYYY)To ____ (MM) _____(DD) _______(YYYY)
Which city/country will you apply for the visa :_____________
Postal address (where to send this I.L.) :_______________
Contact telephone :_______________
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Student travel grants
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Young scientists with an age below 35, who are presenting a paper or poster, can apply for a travel award at the International Association of Geodesy (IAG).The application form with all information can be accessed here.
The deadline for application is 31 July 2018.
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Conference location
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3rd floor of SHAO Building
80 Nandan Road, Shanghai 200030, China
Map of SHAO and Hotels:
Take Metro/Subway to SHAO:
At Pudong International Airport, please take Line 2 to Century Avenue Station (ÊÀ¼o´óµÀÕ¾) and then trasfer line 9 to Xujiahui Station (Ðì¼Ò»ãÕ¾), exit at Gate 1 and then can see SHAO.
At Hongqiao International Airport/train station, please take line 10 to Jiaotong University Station (½»Í¨´óѧվ) and then transfer line 11 with one stop to Xujiahui Station (Ðì¼Ò»ãÕ¾), exit at Gate 1 and then can see SHAO.
Take a taxi to Jianguo Hotel:
Please follow the signs at the airport and find official taxi as well as ask taxi driver to take you to 80 Nandan Road, Shanghai Astronomical Observatory, CAS, Shanghai.£¨Ðì»ãÇøÄϵ¤Â·80ºÅ£¬ÉϺ£ÌìÎĄ̈£©
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Contact information
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Questions on invitation letter and payment, please contact Zhounan Dong (+86-21-15116401991; zndong@shao.ac.cn)
Questions on accomodation reservation, please contact Ke Su (+86-21-17621019466; ksu@shao.ac.cn)
Questions on website and program, please contact Jiandong Liu (+86-21-17765134259; jd_liu@shao.ac.cn)
Questions on exhibition, please contact Lucy Luo (+86-21-13524733078; 2383119084@qq.com)
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Full papers
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Full papers for Remote Sensing Spcial Issue on "Latest Results and Developments in GNSS Ionosphere Theory, Methods, Technologies, Applications and Future Challenges" (SCI/ISI):
All abstracts accepted and presented at the Conference (oral or poster) are welcome to submit as papers for publication in the International Journal of "Remote Sensing" Spcial Issue on GNSS Ionosphere. More submission information can be found at http://www.mdpi.com/journal/remotesensing/special_issues/IWGI_2018
Deadline of full paper submission
30 June 2019
Contacts on full paper submission
M Mainul Hoque (mainul.hoque@dlr.de)
Shuanggen Jin (sgjin@shao.ac.cn)
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《测绘学报》2018年第9期网刊发布
听李德仁、杨元喜、龚健雅三位院士讲述“我的科研故事”
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权威 | 专业 | 学术 | 前沿
2、单亲家庭的男孩子都有哪些心理问题：单亲家庭男孩心理问题
单亲家庭男孩心理问题 篇
1、缺乏安全感。
我见过一个离异家庭的单亲孩子，他曾这样告诉我： “他们之间都可以相互背叛，您觉得我还能靠得住他们吗？”
2、严重的自卑。
我们常见到的现象就是，那些单亲家庭的孩子社交会出问题。性格表现为孤单、内向。这皆是因为有严重的自卑感。自卑的人，做事缺乏信心，同时也缺乏进取心。
3、容易有内疚感。
那些单亲家庭的孩子会无意识地把父母离异的责任自己承担起来，或多或少。这种曲解就会让孩子陷入烦恼，常常自责，内疚感加重。
4、容易变得无情无义。
因为没有一个温馨的、充满爱的家庭环境，孩子时间长了就会变得无情无义。这也是为什么单亲家庭的孩子在外总是惹是生非的一个主要原因。
5、缺乏同情心。
一个孩子长期处在一个“战争”家庭环境中，学会的都是以牙还牙，从而造成同情心的严重缺乏。
6、思想的空虚。
当父母都忙于处理自己焦头烂额的情感的时候，必然会疏于孩子心理成长的管理。那些健康的阳光的思想就会离孩子远去，从而让孩子感觉思想的空虚。
扩展资料
家庭的破裂，仿佛是“天降横祸”，对年幼的孩子来说，他们缺乏必要的心理准备，因而他们遭受的打击比父母更大，而且孩子比大人敏感、脆弱，他们还不具备自我调整心理的能力，一时还难以面对家庭破损的严酷现实，因而会感到无所适从、闷闷不乐。
孩子也懂得比较，他们会拿自己的现在与过去比，感到自己处境已大不如前，拿自己与健全家庭的孩子比，自感不加别人家的孩子，因而滋生出自卑的心理，做事变得胆怯，缺乏自信，缺乏进取和积极向上的精神，而且因为觉得自己不如别人家的孩子。
这些孩子由于被父母所疏远而产生抑郁，不愿意与人接触，对周围的人常有戒备、厌烦的心理表现出神经过敏的症状。他们总怀疑别人会在背后议论自己家庭的缺损和父母的离异，认为别人都瞧不起自己，不愿意向他人敞开自己的心扉，便自我封闭，不愿外出活动，不愿与人打交道，表现出孤独、内向的性格特征。
单亲家庭男孩心理问题 篇
如何正确引导单亲家庭孩子的心理
有些单亲家庭在分解之后，抚养孩子的一方都会拒绝对方去看望自己的子女，孩子的心理会造成很大的影响，也会造成一定的创伤，会给孩子心理上磨灭出仇恨的种子。父母在离婚之后将仇恨直接的转移给自己的孩子，在教育孩子的过程当中，都会说对方的错误能够让孩子远离对方。我孩子从小到大，在和人接触的时候，都会产生一些变态的心理表现。因此父母应该尽最大的努力能够对孩子负起责任，让孩子能够在父母的爱抚当中健康成长。
不要让孩子成为父母离婚的牺牲品，父母之间出现的问题，千万不要强压给自己的子女，更不要去为了满足孩子的种种要求，去讨好孩子的欢心，因为有些父母会认为孩子是负担，或者是在，夫妻离婚之后都会想要孩子，都会极尽可能地使孩子成为自己的牺牲品。孩子就会利用父母之间的力量，控制父母，心理上会变得更加的自私和虚伪在父母彼此竞争当中，孩子也会成为一种牺牲品。
因此，不要让孩子能够去充当另一半的替代角色，因为父母之间的问题并不是孩子所造成的，最好是能够让孩子茁壮的成长是孩子的心理不会受到影响，应该多去鼓励孩子参加一些集体的活动。父母之间应该相互的进行尊重，让孩子能够去感受到家庭的和谐气氛，让孩子能够变得更加的心情舒畅和开朗，小孩子的兴趣和爱好，包括乐器和唱歌以及绘画，能够从单亲家庭造成的阴影当中走出来。
单亲家庭男孩心理问题 篇
1、缺乏安全感。
我见过一个离异家庭的单亲孩子，他曾这样告诉我： “他们之间都可以相互背叛，您觉得我还能靠得住他们吗？”
2、严重的自卑。
我们常见到的现象就是，那些单亲家庭的孩子社交会出问题。性格表现为孤单、内向。这皆是因为有严重的自卑感。自卑的人，做事缺乏信心，同时也缺乏进取心。
3、容易有内疚感。
那些单亲家庭的孩子会无意识地把父母离异的责任自己承担起来，或多或少。这种曲解就会让孩子陷入烦恼，常常自责，内疚感加重。
4、容易变得无情无义。
因为没有一个温馨的、充满爱的家庭环境，孩子时间长了就会变得无情无义。这也是为什么单亲家庭的孩子在外总是惹是生非的一个主要原因。
5、缺乏同情心。
一个孩子长期处在一个“战争”家庭环境中，学会的都是以牙还牙，从而造成同情心的严重缺乏。
6、思想的空虚。
当父母都忙于处理自己焦头烂额的情感的时候，必然会疏于孩子心理成长的管理。那些健康的阳光的思想就会离孩子远去，从而让孩子感觉思想的空虚。
扩展资料
家庭的破裂，仿佛是“天降横祸”，对年幼的孩子来说，他们缺乏必要的心理准备，因而他们遭受的打击比父母更大，而且孩子比大人敏感、脆弱，他们还不具备自我调整心理的能力，一时还难以面对家庭破损的严酷现实，因而会感到无所适从、闷闷不乐。
孩子也懂得比较，他们会拿自己的现在与过去比，感到自己处境已大不如前，拿自己与健全家庭的孩子比，自感不加别人家的孩子，因而滋生出自卑的心理，做事变得胆怯，缺乏自信，缺乏进取和积极向上的精神，而且因为觉得自己不如别人家的孩子。
这些孩子由于被父母所疏远而产生抑郁，不愿意与人接触，对周围的人常有戒备、厌烦的心理表现出神经过敏的症状。他们总怀疑别人会在背后议论自己家庭的缺损和父母的离异，认为别人都瞧不起自己，不愿意向他人敞开自己的心扉，便自我封闭，不愿外出活动，不愿与人打交道，表现出孤独、内向的性格特征。
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