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蛞蝓是什么动物,蛞蝓是什么动物类型(GNSS电离层国际研讨会)

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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

蛞蝓是什么动物,蛞蝓是什么动物类型(GNSS电离层国际研讨会)

◆◆

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


    ◆◆

    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


    ◆◆

    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

    ◆◆

    Abstract submission

    ◆◆



    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: _______________


    ◆◆

    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)

    ◆◆

    Participants

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NumberNAMEAFFILIATIONCOUNTRYABSTRACTEMAIL
1Libo Liu Institute of Geology and Geophysics, CASChinaIonospheric monitoring and physics: Recent progresses in China liul@mail.iggcas.ac.cn
2Norbert Jakowski/M. Mainul Hoque German Aerospace Center (DLR)GermanyFast and improved ionospheric correction by NTCM models using GNSS broadcast coefficients
The Nighttime Winter Anomaly (NWA) effect - a persistent feature of the mid-latitude ionospheres at the American and Asian longitude sectors
Norbert.Jakowski@dlr.de
3Volkan Akgul Bulent Ecevit UniversityTurkeyHigh-order ionopsheric effects on GPS-estimated tropospheric delay gradients akgulvo@gmail.com
4Manuel 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.com
6Shuanggen Jin Shanghai Astronomical Observatory, CASChinaGNSS cloudy platform for digital space: Advances, applications and opportunities sgjin@shao.ac.cn
7Y. Tony Song NASA JPLUSAxxxTony.Song@jpl.nasa.gov
8Xiaodong Qian Shanghai Astronomical Observatory, CASChinaIonospheric delay correction for mean sea level change from CYGNSS GNSS-R observations xdqian@shao.ac.cn
9Mainul Hoque German Aerospace Center (DLR)GermanyEstimates of higher order ionospheric effects for GNSS signals received onboard LEO satellites Mainul.Hoque@dlr.de
10Andres Calabia Shanghai Astronomical Observatory, CASChinaVariations of thermospheric air mass density derived from GRACE accelerations and GPS POD andres@calabia.com
11Jiandong Liu Shangha Astronomical Observatory, CASChinaWave distribution and activities in the upper Mars atmosphere from multi-satellite accelerometer observations jd_liu@shao.ac.cn
12Jens Berdermann German Aerospace Center (DLR)GermanyxxxJens.Berdermann@dlr.de
13Jiuhou Lei University of Science and Technology of ChinaChinaxxxleijh@ustc.edu.cn
14Ke Su Shanghai Astronomical Observatory, CASChinaEvaluation of ionospheric ionospheric effects on multi-GNSS PPP performances ksu@shao.ac.cn
15Yuichi Otsuka Nagoya UniversityJapanxxxotsuka@isee.nagoya-u.ac.jp
16Liangliang Yuan Shanghai Astronomical Observatory, CASChinaThermospheric mass density variations following the September 2017 geomagnetic storm from GRACE and SWARM precise orbits 18905648099@189.cn
17Xin Liu Shanghai University & SHAOChinaIonospheric disturbances following the 2011 Tohoku-Oki Tsunami from GPS observations 990528837@qq.com
18Chao Gao Shanghai Astronomical Observatory, CASChinaHigh-order ionospheric effects on neutral atmospheric parameters estimation from FY-3C GPS Radio Occultation 349827456@qq.com
19Zhonnan Dong Shanghai Astronomical Observatory, CASChina3-D water vapor tomography in Wuhan from GPS, BDS and GLONASS observations zndongcsu@163.com
20Charles Lin National Cheng Kung UniversityTaiwan, Chinaxxxcharles@mail.ncku.edu.tw
21Ershen Wang Shenyang Aerospace UniversityChinaSatellite Selection Algorithm for Multi-constellation GNSS Positioning wanges_2016@126.com
22Yuhan Liu Shanghai University & SHAOChinaIonospheric disturbances following the 2018 Mw=7.9 Alaska earthquake from GPS observations inuyasha471@qq.com
23Dasari 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.com
24Dasari 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.com
25Virendra Patel Sardar Vallabhbhai National Institute of TechnologyIndiaImpact of ockhi cyclone on IRNSS/NavIC GNSS signal due to ionospheric and tropospheric variation virendra369@gmail.com
26Gopal Mondal Jadavpur UniversityIndiaIonospheric variation during El Nino and La Nina years over tropical Pacific Ocean gopalmondal18@gmail.com
27Feza Arikan Hacettepe UniversityTurkeyPerformance of IRI-Plas with GIM-TEC input as Compared to Ionosonde Data for Equinox Seasons arikan@hacettepe.edu.tr
28Solen Kumbay Yildiz Hacettepe UniversityTurkeyInvestigation of Spatio-Temporal Variability of Midlatitude Ionosphere Using GIM-TEC solen@ee.hacettepe.edu.tr
29K.D.Sriniuasu Vadlamurt Andhra UniversityIndiavkdsrinivasu@gmail.com
30Yue 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.edu
31Haiyang Fu Fudan University Chinafuhaiyang@gmail.com
32Yanhong Chen National space science center,CAS ChinaIonosphere modeling, specification and application from GNSS observation chenyh@nssc.ac.cn
33Shun 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.edu
41Wenfeng 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.com
53Yangyi Sun China University of Geosciences (Wuhan) ChinaEl Nino - Southern Oscillation signature in ionosphere observed by FORMOSAT-3/COSMIC radio occultation sunyy@cug.edu.cn
54Kunpeng 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.com
55Jun Chen School of Geodesy and Geomatics, Wuhan University ChinaModeling and analysis of a new ionospheric mapping function cj_snake@whu.edu.cn
56Hongda Miao Xidian University ChinaA GPU Model of the Ionosphere Based on Sami2 1925059579@qq.com
57Hongda Miao Xidian University ChinaA GPU Model of the Ionosphere Based on Sami2 1925059579@qq.com
58XiangXiang 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.com
59Yongxing Zhu Information Engineering University ChinaAccuracy analysis of broadcasting ionospheric parameters for the latest BDS-3 experimental satellites 18049269002@126.com
60Weijun Lu National Astronomical Observatories, CAS ChinaA preliminary result of ionospheric TEC derivation from GPS carrier phase observations luweijun14@mails.ucas.ac.cn
61Guoqiang Pang University Of Electronic Science And Technology Of China ChinaA new study of ionospheric delay based on dual-frequency BeiDou reference station GuoqiangPang15@163.com
62Conglin Zhou Geomatic Center of Guangxi ChinaAnalysis of the application of GNSS technology in seismic research 573014033@qq.com
63Jinghua Li National Astronomical Observatories, CAS ChinaEvaluation of the Klobuchar model in TaiWan jhli@nao.cas.cn
64Shuaimin Wang Institute of Space Science, Shandong University ChinaEstablishment of weighted mean temperature model in the polar region wsm1949@sina.com
65Biao Jin Institute: Space star technology co., LTD ChinaSBAS Ionospheric Spatial Threat Model and the Integrity in China Area 617630427@qq.com
66Mingzhe Li Institute of Geology and Geophysics, CAS ChinaCharacterization of the residual ionospheric errors in neutral radio occultation retrievals limingzhe@mail.iggcas.ac.cn
67Mingzhe Li Institute of Geology and Geophysics, CAS ChinaCharacterization of the residual ionospheric errors in neutral radio occultation retrievals limingzhe@mail.iggcas.ac.cn
68Hang Liu Xi'an University of Science and Technology Chinaxx673290038@qq.com
69Xiaohua 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.cn
70Jinmei 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.com
71Yue 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.com
72Xinying Zhong Geomatic Center of Guangxi ChinaPERFORMANCE ANALYSIS OF BEIBU GULF OF GUANGXI BEIDOU NAVIGATION GROUND-BASED AUGMENTATION SYSTEM 351942387@qq.com
73Yong 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.it
78Takashi MARUYAMA National Astronomical Observatories, CAS
National Institute of Information and Communications Technology
China/JapanPrecise estimation of total electron content by double thin-shell model at equatorial and low latitudes using local receiver network tmaru@nict.go.jp
79Jinghua Li National Astronomical Observatories, CAS ChinaEvaluation of the Klobuchar model in TaiWan jhli@nao.cas.cn
80Ning 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.com
81Jinyun Guo Shandong University of Science and TechnologyChinaxxjinyunguo1@126.com
82Shunrong Zhang MIT Haystack ObservatoryUSAThe 2017 Great America Eclipse induced ionospheric bow waves shunrong@mit.edu
83Jianfeng Li School of Earth Science and Environmental Engineering, Southwest Jiaotong UniversityChinaCoupling Characteristics analysis for Ionospheric Storm and Geomagnetic Storm jianfengli@my.swjtu.edu.cn
84Guanyi 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.cn
85Chao Xiong GFZ German Research Centre for Geosciences PotsdamGermanyThe GPS signal interruption of Swarm satellites caused by ionospheric plasma irregularities bear@gfz-potsdam.de
86Shunzu Gao Electronic Information School, Wuhan UniversityChinaIntegrated Algorithm for TEC Measurement with GPS and BDS Receivers gaoshz@whu.edu.cn
87Kaixuan 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.com
88Yufei Wu University Of Electronic Science And Technology Of China ChinaIonospheric Disturbance Monitoring Based on Convolution Neural Networks 120020435@qq.com
89zhengxie Zhang University Of Electronic Science And Technology Of China ChinaReal-Time Extracting Ionospheric Delays and Establishing Regional Model by CORS 15651975330@163.com
90Guangyuan 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.com
91Weihua Bai National Space Science Center, Chinese Academy of Sciences ChinaThe validation and application of ionospheric radio occultation products derived from FY3C/GNOS bjbwh@163.com
92Guozhu 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.cn
93Jieqing 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.cn
94Wenxiang Li Research Institute of Electronic Science and Technology, UESTC ChinaReview of Ionospheric TEC and NmF2 Perturbations Before Wenchuan Earthquake LWX_UESTC@163.com
95Shenwei Shi Nanjing University of Information Science & Technology Chinaxxt1142430226@163.com
96Jiabing Guo Nanjing University of Information Science & Technology Chinaxx1292196066@qq.com
97Yiduo Wen Nanjing University of Information Science & Technology Chinaxx1505006362@qq.com
98Naifeng Fu Shanghai Astronomical Observatory, CAS Chinaxxnffu@shao.ac.cn
99Peng Guo Shanghai Astronomical Observatory, CASChinaxxxgp@shao.ac.cn
100Mengjie Wu Shanghai Astronomical Observatory, CASChinaxxxmjwu@shao.ac.cn
101Sergey Pulinets Space Research Institute, RASRussiaxxxpulse1549@gmail.com
102Hui Qiu Shanghai Astronomical Observatory, CASChinaxxxws2834825886@163.com
103Michael Schmidt Technische Universitat Munchen (TUM)Germanyxxxmg.schmidt@tum.de
104Zhaoyang Hong ShanghaiTech University & SHAOChinaxxx504218720@qq.com
105Jie Chen Xiangtan University & SHAOChinaxxx422061442@qq.com
106Andrzej Krankowski University of Warmia & Mazury in OlsztPolandxxxkand@uwm.edu.pl
107Qiang Chen Xiangtan University & SHAOChinaxxx422061442@qq.com
108Wei Shang Shanghai University & SHAOChinaxxx90791215@qq.com
109Zengji Zheng Shanghai Astronomical Observatory, CASChinaxxx13488316276@126.com
110Bahruz Ahadov Shanghai Astronomical Observatory, CASChinaxxxgeofizik608@mail.ru
111Shuhua Ye Shanghai Astronomical Observatory, CASChinaxxxysh@shao.ac.cn
112Yang Yu Shanghai Astronomical Observatory, CASChinaxxxyuyang@shao.ac.cn
113Qinyun Zhang Shanghai University & SHAOChinaxxx915424294@qq.com
114Oufang Luo Shanghai Astronomical Observatory, CASChinaxxxofluo@hotmail.com
115Xiaojuan Tian Shanghai Astronomical Observatory, CASChinaxxxxjtian@shao.ac.cn
116Xuerui Wu Shanghai Astronomical Observatory, CASChinaxxxxrwu@shao.ac.cn
117Mostafa S. Abd-Elbaky Shanghai Astronomical Observatory, CASChinaxxxmstabdelbaky@gmail.com
118Sheng Liu XAO/SHAO, CASChinaxxxliusheng17@mails.ucas.ac.cn
119Hugo Carreno-Luengo Centre Tecnologic de Telecomunicacions de Catalunya (CTTC)Spainxxxhugo.carreno.luengo@gmail.com
120Chun Li Xiangtan University & SHAOChinaxxx422061442@qq.com
121Yang He Shanghai University & SHAOChinaxxx1137353689@qq.com
122Hong Lu Institute of High Energy Physics,CASChinaxxluh@ihep.ac.cn
123Ming Ou China Research Institute of Radiowave PropagationChinaxxohm1122@163.com
124Jian 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


  • ◆◆

    inviation&visa

    ◆◆


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 :_______________

◆◆

Student travel grants

◆◆

    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.

    ◆◆

    Conference location

    ◆◆


  • 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£©


    ◆◆

    Contact information

    ◆◆

  • 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)


    ◆◆

    Full papers

    ◆◆

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)

蛞蝓是什么动物,蛞蝓是什么动物类型(GNSS电离层国际研讨会)蛞蝓是什么动物,蛞蝓是什么动物类型(GNSS电离层国际研讨会)蛞蝓是什么动物,蛞蝓是什么动物类型(GNSS电离层国际研讨会)

《测绘学报》2018年第9期网刊发布

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2、蛞蝓是什么动物

蛞蝓是什么动物

蛞蝓是软体动物,蛞蝓,腹足纲,柄眼目,蛞蝓科。又称水蜒蚰,中国南方某些地区称蜒蚰(不是蚰蜒),俗称鼻涕虫,是一种软体动物,与部分蜗牛组成有肺目。

蛞蝓是腹足纲(Gastropoda)中壳退化的软体动物。壳可退化为一体内片状结构,成一列颗粒,或完全消失。有的危害园林。肺螺亚纲(Pulmonata)俗称蛞蝓,其体软,有黏液,生活在潮湿的场所(淡水产者仅知一种)。温带地区常见的阿勇蛞蝓科(Arionidae)、蛞蝓科(Limacidae)和嗜黏液蛞蝓科(Philomycidae)的种类取食真菌和腐叶。

蛞蝓是什么样的动物?

鼻涕虫”俗名“蜒蚰”,由蜗牛转变而来,现生种类广分布于欧洲、亚洲、北美和北非。陆生。体柔软,形状似去壳的蜗牛,外形呈不规则的圆柱形。壳退化为一石灰质的薄板,位于身体前端背部,被外套膜包裹而成内壳。有尾嵴。体呈灰色、黄褐色或橙色,具有不明显的暗带和斑点。触角2对。眼位于后触角的顶端。雌、雄生殖孔为1共同孔,位于身体右侧、前右触角的后下方。肺孔开口在外套膜的后缘。身体经常分泌粘液,爬行后留下银白色的痕迹。生活于阴暗、潮湿处,白昼潜伏,夜晚和雨天外出活动。雌雄同体,交尾产卵,卵产于潮湿的土壤中。取食植物的嫩叶嫩芽,为蔬菜、果树、烟草、棉花等的敌害。中国常见的种类有黄蛞蝓。大型,伸展时体长可达120毫米。体黄褐色或深橙色,有浅黄色斑点。生活在阴暗潮湿的地方或住宅的阴暗处。在高湿、高温的季节最为活跃。喜食植物,为农业的害虫。

蛞蝓是什么虫?

蛞蝓 [kuò yú](学名 Agriolimax agrestis Linnaeus)为腹足纲,柄眼目,蛞蝓科动物的统称。中国南方某些地区称蜒蚰(不是蚰蜒),俗称鼻涕虫,是一种软体动物,与部分蜗牛组成有肺目。雌雄同体,外表看起来像没壳的蜗牛,体表湿润有黏液,民间流传在其身上撒盐使其脱水而死的捕杀方法的确有用。

常见蛞蝓像没有壳的蜗牛。成虫伸直时体长30~60毫米,体宽4~6毫米;内壳长4毫米,宽2.3毫米。长梭型,柔软、光滑而无外壳,体表暗黑色、暗灰色、黄白色或灰红色。触角2对,暗黑色,下边一对较短,约1毫米,称前触角,有感觉作用;上边一对长约4毫米,称后触角,端部具眼。口腔内有角质齿舌。体背前端具外套膜,为体长的1/3,边缘卷起,其内有退化的贝壳(即盾板),上有明显的同心圆线,即生长线。同心圆线中心在外套膜后端偏右。呼吸孔在体右侧前方,其上有细小的色线环绕。崎钝。粘液无色。在右触角后方约2毫米处为生殖孔。卵椭圆形,韧而富有弹性,直径2~2.5毫米。白色透明可见卵核,近孵化时色变深。幼虫初孵体长2~2.5毫米,淡褐色,体形同成体。

本文关键词:蛞蝓是什么动物有害吗,蛞蝓对人体有什么危害,蛞蝓是什么动物类群,蛞蝓怎么读,蛞蝓是什么动物值钱吗。这就是关于《蛞蝓是什么动物,蛞蝓是什么动物类型(GNSS电离层国际研讨会)》的所有内容,希望对您能有所帮助!更多的知识请继续关注《犇涌向乾》百科知识网站:http://www.029ztxx.com!

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