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Entry ID: CN_NADC_2016_Arctic_Yellow_River_Station_unicore_spring
Publish Date: 2017-07-04
Author: An Jiachun
Keywords: huanghe Station, GPS
Dataset: Files(1) Filesize(2.7 MB)
Summary: In spring of 2016, the geodetic GPS receiver is used to collect the GPS observations.The types of GPS observations are dual frequency pseudorange and dual frequency carrier phase. the place is Yellow River Station. the time is spring, 2016. one observation file one day, duration is 24 hours. the receiver is UNICORE UB4B0I, the antenna is NOV750. the sample rate is 60 seconds. the file format is Hatanaka RINEX. the precision is 1cm in horizontal direction and 2cm in vertical direction. The proper data processing softwares contain GAMIT and LGO. The proper data processing modes contain PPP and DGPS.
Entry ID: CN_NADC_2014_Arctic_Yellow_River_Station_unicore_autumn
Publish Date: 2017-07-04
Author: An Jiachun
Keywords: huanghe Station, GPS
Dataset: Files(1) Filesize(2.3 MB)
Summary: In autumn 2014, the geodetic GPS receiver is used to collect the GPS observations.The types of GPS observations are dual frequency pseudorange and dual frequency carrier phase. the place is Yellow River Station. the time is autumn, 2014. one observation file one day, duration is 24 hours. the receiver is UNICORE UB4B0I, the antenna is NOV750. the sample rate is 60 seconds. the file format is Hatanaka RINEX. the precision is 1cm in horizontal direction and 2cm in vertical direction. The proper data processing softwares contain GAMIT and LGO. The proper data processing modes contain PPP and DGPS.
Entry ID: CN_NADC_2012_Antarctic_GreatWall_WLR7_Tide
Publish Date: 2013-11-15
Author: Ai Songtao
Keywords: Tide Gauge, Great Wall Station
Location: GreatWallStation
Dataset: Files(1) Filesize(8.5 MB)
Summary: In 2012 January China Antarctic Great Wall Station with the annual running of the tide station by Wuhan University. The type of instruments is WLR7 from Norwegian Aanderaa company. The precision of WLR7 is up to mm, and the data can be acquired via a cable connecting the sensor and deck unit in real time measurement.The tide data automatic daily return and preliminary analysis of post. Those data sets were the tide gauge data acquired from 2012 to 2016 at Great Wall Station.There is not data collected in 2013 due to cable damage.
Entry ID: CN_NADC_2011_Antarctic_Zhongshan_WLR7_tide
Publish Date: 2013-11-15
Author: Ai Songtao
Keywords: Zhongshan Station, Tide Gauge
Dataset: Files(1) Filesize(5.1 MB)
Summary: Tide gauge data at Chinese Antarctic Zhongshan Station in from 2010 to 2012 by Wuhan University.The type of instruments is WLR7 from Norwegian Aanderaa company. The precision of WLR7 is up to mm, and the data can be acquired via a cable connecting the sensor and deck unit in real time measurement.Due to cable damage, there were no data from 2013 to 2015.New instrument RBR from Canada was set up in 2016.
Entry ID: CN_NADC_2016_Area_Zhongshan_Station_Sensor_Description
Publish Date: 2017-05-15
Author:
Keywords: Declination, Horizontal Intensity, Vertical Intensity, Inclination, Total Intensity
Dataset: Files(1) Filesize(10.7 MB)
Summary: Geomagnetics and upper atmosphere dynamics are subjects which based on observation. The long term data acquisition has not only significant to basic research about the space physics, but also has many applications in national defense and national economy as well. Furthermore, the Antarctic geomagnetic and space environmental observation play an important role in the meridian observation chain of space physics in China. The observation contains: geomagnetic relative variations (three components H, D and Z), absolute observation (three components D, I and F), geomagnetic pulsation, ionospheric scintillation and TEC observation etc. In addition, data processing must be carried out everyday, and daily instrument maintenance is necessary. Main observation instruments are as follows: 1.G856 proton magnetometer 2.CTM-DI variometer 3.MD style digital data acquisition system 4.Digital geomagnetic pulsation variometer 5.VLF receiver 6.GSV4004 ionospheric scintillation and TEC monitor
Entry ID: CN_NADC_2014_Great_Wall_station_Great_Wall_Station_CMG-3ESP_Description
Publish Date: 2015-05-09
Author: Chang Lijun
Keywords: Great Wall Seismic Station, seismic data
Dataset: Files(0) Filesize(0 字节)
Summary: Seismic data observed at the Great Wall Station was collected during the 30th Chinese Antarctic expedition in 2014. Data-collection process follow New Manual of Seismological Observatory Practice.
Entry ID: CN_NADC_2016_Antarctic_Great_Wall_Station_CMG-3ESP_Description
Publish Date: 2017-03-23
Author: Chang Lijun
Keywords: seismic data, Great Wall Seismic Station
Dataset: Files(0) Filesize(0 字节)
Summary: Seismic data observed at the Great Wall Station was collected during the 32th Chinese Antarctic expedition. Data-collection process follow New Manual of Seismological Observatory Practice.
Entry ID: CN_NADC_2015_Antarctic_Chinese_Antarctic_Great_Wall_Station_CMG-3ESP_Description
Publish Date: 2017-03-23
Author: Chang Lijun
Keywords: seismic data, Great Wall Seismic Station
Dataset: Files(0) Filesize(0 字节)
Summary: Seismic data observed at the Great Wall Station was collected during the 31th Chinese Antarctic expedition in 2015. Data-collection process follow New Manual of Seismological Observatory Practice.
Entry ID: CN_NADC_2015_Antarctic_Chinese_Antarctica_Zhongshan_Station_CCD_IMAGER_Description
Publish Date: 2016-12-18
Author: Huang Dehong
Keywords: All-sky Aurora Image, Zhongshan Station
Dataset: Files(0) Filesize(0 字节)
Summary: The multiple wavelength all-sky aurora imager is to detect all-sky auroral morphology with multiple wavelength bands at extreme low light conditions.
Entry ID: CN_NADC_2014_2015_Ross_Sea_Inexpressible_Island_zy-3_Description
Publish Date: 2017-01-06
Author: Wang Lianzhong
Keywords: subglacial topography, topographic survey
Dataset: Files(0) Filesize(0 字节)
Summary: Complete the 1:50000 topography map of key inspection area in Vitoria using the stereo mapping without ground control based on the remote sensing satellite data of ZY-3,integrated LIMA DOM and ASTER GDEM and other supplementary information