Search Help
Did you find what you were looking for? Yes No
Thumbnail Icon [Originating_Center='Polar Research Institute of China']


Refine by Category
 
Refine by Full text

 

60 Titles Match Your Query
Showing 1 through 50 of 60 Next
1. Raw data of XBT and XCTD by the 18th CHINARE in 2001-2002 [2001-2002_18-18_S_OC_OC02_SA_O070200_001_R0_Y]
This raw data of MAKE IIIC-CTD was been collected in Prydz Bay region of the Southern Ocean during the austral summer of 2001/2002.


2. All-Sky TV Camera Data at Zhongshan Station, Antarctica, Year 2002 dataset - CNNADC_2002_18_S_ASC [CNNADC_2002_18_S_ASC]
All-sky TV camera is to monitor auroral displays nearly 180 degrees in filed of view, it consists of all-sky camera, control box, timing generator, timer corrector, two VHS recorders, SVHS recorders ...


3. Weather Data of the 22nd Voyage of Chinese Antarctic Research in 2005/2006 - CN_NADC_2005_2006_Pac_Ind_Atl_Polar_regions_Location_MILOS500_Description [CN_NADC_2005_2006_Pac_Ind_Atl_Polar_regions_Location_MILOS500_Description]
During the 22nd voyage of Chinese Antarctic Research Expedition in 2005/2006, we use automatic station vaisala 500 to get the weather information, including: DATE, TIM, LAT, LON, T(c) (AVE, MAX, MIN), ...


4. Weather Data of the 24th Voyage of Chinese Antarctic Research in 2007/2008 - CN_NADC_2007_2008_Pac_Ind_Atl_Polar_regions_Location_MILOS500_Description [CN_NADC_2007_2008_Pac_Ind_Atl_Polar_regions_Location_MILOS500_Description]
During the 24th voyage of Chinese Antarctic Research Expedition in 2007/2008,we use automatic station vaisala 500 to get the weather information, including: DATE, TIM, LAT, LON, T(c) (AVE, MAX, MIN), ...


5. Weather Data of the 25th Voyage of Chinese Antarctic Research in 2008/2009 - CN_NADC_2008_2009_Area_Antarctica_MILOS500_Description_weatherdata [CN_NADC_2008_2009_Area_Antarctica_MILOS500_Description_weatherdata]
During the 25th voyage of Chinese Antarctic Research Expedition in 2008/2009, we use automatic station vaisala 500 to get the weather information, including: DATE, TIM, LAT, LON, T(c) (AVE, MAX, MIN), ...


6. Weather Data of the 26th Voyage of Chinese Antarctic Research in 2009/2010 [CN_NADC_2009_2010_Area_Location_SensorName_Description]
During the 26th voyage of Chinese Antarctic Research Expedition in 2009/2010,we use automatic station vaisala 500 to get the weather information, including: DATE, TIM, LAT, LON, T(c) (AVE, MAX, MIN), ...


7. 1998-1999 Raw data of CTD in Prydz Bay region of the southern Indian Ocean, CHINARE-15 [1998-1999_15-15_S_OC_OC05_LO_O011301_000_R0_Y]
A series of measurements in water temperature, conductivity and depth was carried out during the austral summer of 1998/99 within and the north of Prydz Bay, the southern Indian Ocean.34 oceanographic ...


8. 1999-2000 Raw data of CTD in Prydz Bay region of the southern Indian Ocean, CHINARE-16 [1999-2000_16-16_S_OC_OC05_LO_O011301_000_R0_Y]
A series of measurements in water temperature, conductivity and depth was carried out during the austral summer of 1999/2000 within and the north of Prydz Bay, the southern Indian Ocean.44 oceanographic ...


9. All-Sky TV Camera Data at Zhongshan Station, Antarctica, Year 2001 dataset [CNNADC_2001_17_S_ASC_GW]
All-sky TV camera is to monitor auroral displays nearly 180 degrees in filed of view, it consists of all-sky camera, control box, timing generator, timer corrector, two VHS recorders, SVHS recorders ...


10. All-Sky TV Camera Data at Zhongshan Station, Antarctica, Year 2004 dataset [CNNADC_2004_ZhongshanStation_Antarctica_ASC_Dataset]
All-sky TV camera is used to monitor aurora display nearly 180 degrees in filed of view, it consists of an all-sky camera,a control box, a timing generator, a time corrector, two HD-DVD recorders ...


11. All-Sky TV Camera Data at Zhongshan Station, Antarctica, Year 2005 dataset [CNNADC_2005_Zhongshan_Station_Antarctica_ASC_Description]
All-sky TV camera is to monitor auroral displays nearly 180 degrees in filed of view, it consists of all-sky camera, control box, timing generator, timer corrector, two VHS recorders, SVHS recorders ...


12. Data of biodiversity of marine bacterioplankton at Kongsfjorden in the summer of 2008 [CNNADC_2008_King_Bay_Polar_regions_SensorNameBacterial_diversity]
Phylogenetic diversity of the marine bacterioplankton in Kongsfjorden (Spitsbergen) was investigated through 16S rRNA gene analysis. Community fingerprint analysis by PCR-denaturing gradient gel electrophoresis ...


13. Data of isolation and identification of Actinobacteria from rhizospheric soil collected from the Arctic Yellow River Station in 2007 [CNNADC_2007_King_Bay_Kongsfjorden_SensorName_Description]
Using spread-plate technique, actinobacterial strains were isolated from rhizospheric soil of 7 plants collected in the Arctic Yellow River Station, New Alesund, Svalbard (Ny-Alesund, the Arctic). ...


14. Data of nutrients and DO concentration in Prydz Bay during the 24th CHINARE, 2007-2008 [CNNADC_2008_Prydz_Bay_Southern_Ocean_SensorName_Description]
The distribution and concentration of nutrients, including phosphate, nitrate, nitrite, ammonium and silicate were investigated in the Prydz Bay East Antarctica during CHINARE-24. The results show ...


15. Data set of Imaging Riometer at Zhongshan Station, Antarctica, Year 2002 [CNNADC_S2002_S_IR_ZS]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300×300 ...


16. Data set of Imaging Riometer at Zhongshan Station, Antarctica, Year 2004 [CNNADC_2004_200132366531449_2133526497_IMAGING_RIOMETERS_Dataset]
The Imaging Riometer is used to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of ...


17. Data set of Imaging Riometer at Zhongshan Station, Antarctica,Year 2000 [2000_16-16_S_ZS_ME01_LO_O024301_001_R0_Y]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300×300 ...


18. Data set of Imaging Riometer during the 17th CHINARE in 2000-2001 [2000-2000_17-17_S_ZS_ME01_LO_O024301_001_R0_Y]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300×300 ...


19. Data set of the ocean surface temperature and salinity in the cruise of the 7th Chinese Antarctic Research Expedition in 1990/1991 [1990-1991_07-07_S_OC_OC02_XX_A058701_001_R0_Y]
From December of 1990 to April of 1991, we surveyed the ocean surface temperature and salinity in the cruise of the 7th Antarctic Scientific Expedition of China.BMT is the Beijing Mean Time.


20. Data set of the ocean surface temperature and salinity in the cruise of the 8th Chinese Antarctic Research Expedition in 1991/1992 [1991-1992_08-08_S_OC_OC02_XX_A059601_001_R0_Y]
From December of 1991 to March of 1992, we surveyed the ocean surface temperature and salinity in the cruise of the 8th Antarctic Scientific Expedition of China.Total 3 cruises were investigated:Shanghai-Hobart,Hobart-Prydz ...


21. Data set of the ocean surface temperature and salinity in the cruise of the 9th Chinese Antarctic Research Expedition in 1992/1993 [1992-1993_09-09_S_OC_OC02_LO_A059601_001_R0_Y]
From November of 1992 to April of 1993, we surveyed the ocean surface temperature and salinity in the cruise of the 9th Antarctic Scientific Expedition of China.


22. Dataset of CTD, XBT and XCTD from the Nth Chinese Antarctic and Arctic Research Expedition, Year 1984-2005 [CNNADC_1984652932005_Polar_Location_CTD_XBTXCTD]
Datasets of CTD, XBT,and XCTD are from the Nth Chinese Antarctic and Arctic Research Expedition from 1984 to 2005. Datasets are available, total 667MB.NADC provides copy by offline.


23. Digisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica ,Year 2001 [CNNADC_2001_S_DPS4_ZS]
The DPS-4, developed by the University of Massachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


24. Digisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica, Year 1998 [CNNADC_S1998_S_DPS4_ZS]
The DPS-4, developed by the University of Masachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


25. Digisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica, Year 2000 [CNNADC_S2000_S_DPS4_ZS]
The DPS-4, developed by the University of Masachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


26. Digisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica, Year 2004 [CNNADC_2004_200132366531449_2133526497_DPS_Dataset]
The DPS-4, developed by the University of Massachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


27. Digisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica, Year 2005 [CNNADC_2005_Zhongshan_Station_Antarctica_DPS_Description]
The DPS-4, developed by the University of Massachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


28. Digisonde Portable Sounder 4 data on the Zhongshan station, Antarctica, Year 1995 [1995_11-11_S_ZS_GP01_LO_O012701_001_R0_Y]
The DPS-4, developed by the University of Masachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


29. Digisonde Portable Sounder 4 data on the Zhongshan station,Antarctic,Year 1996 [1996_12-12_S_ZS_GP01_LO_O012701_001_R0_Y]
The DPS-4, developed by the University of Masachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


30. Digisonde Portable Sounder 4 data on the Zhongshan station,Antarctic,Year 1997 [1997_13-13_S_ZS_GP01_LO_O012701_001_R0_Y]
The DPS-4, developed by the University of Masachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...


31. Fluxgate Magnetometer Data at Zhongshan Station, Antarctic,Year 2002 [CNNADC_S2002_S_FM_ZS]
The Fluxgate magnetometer is to measure relative geomagnetic variations at 3 dimensions, i.e., x, y and z components.The data is recorded on MO disks with two copies, one for Polar Research Institute ...


32. Fluxgate Magnetometer Data at Zhongshan Station, Year 2005 [CNNADC_2005_Zhongshan_Station_Antarctica_FM_Description]
The Fluxgate magnetometer is to measure relative geomagnetic variations at 3 dimensions, i.e., x, y and z components.The data is recorded on MO disks with two copies, one for Polar Research Institute ...


33. Fluxgate Magnetometer Data at Zhongshan Station,Antactic,Year 2001 [CNNADC_S2001_S_FM_ZS]
The Fluxgate magnetometer is to measure relative geomagnetic variations at 3 dimensions, i.e., x, y and z components.The data is recorded on MO disks with two copies, one for Polar Research Institute ...


34. Imaging Riometer Data at Zhongshan Station, Antarctica, Year 2005 [CNNADC_2005_Zhongshan_Station_Antarctica_IMAGING_RIOMETERS_Description]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300×300 ...


35. Induction Magnetometer Data at Zhongshan Station, Antarctica Year 2001 [CNNADC_S2001_S_PM_ZS]
The pulsation magnetometer is to measure D and H components of geomagnetic induction variations. As a cooperation project with Newcastle University, Austrilia. The data is shared by boths sides. The ...


36. Induction Magnetometer Data at Zhongshan Station, Antarctica, Year 2004 [CNNADC_2004_ZhongshanStation_Antarctica_PM_Dataset]
The pulsation magnetometer is used to measure D and H components of geomagnetic induction variations. It is a cooperation project with Newcastle University, Australia. The data is shared by boths ...


37. Induction Magnetometer Data at Zhongshan Station, Antarctica, Year 2005 [CNNADC_2005_Zhongshan_Station_Antarctica_PM_Description]
The pulsation magnetometer is to measure D and H components of geomagnetic induction variations. As a cooperation project with Newcastle University, Australia. The data is shared by both sides. The ...


38. Induction Magnetometer Data at Zhongshan Station, Antarctica,Year 2002 [CNNADC_S2002_S_PM_ZS]
The pulsation magnetometer is to measure D and H components of geomagnetic induction variations. As a cooperation project with Newcastle University, Austrilia. The data is shared by boths sides. The ...


39. Meridian Scanning Photometer Data at Zhongshan Station, Antarctica, Year 2001 [CNNADC_S2001_S_MSP_ZS]
The Auroral Meridian Scanning Photometer is to measure the absolute intensity of aurora brightness along the geomagnetic meridian line. At present the MSP records three wavelengths of auroral emissions ...


40. Meridian Scanning Photometer Data at Zhongshan Station, Antarctica, Year 2002 [CNNADC_S2002_S_MSP_ZS]
The Auroral Meridian Scanning Photometer is to measure the absolute intensity of aurora brightness along the geomagnetic meridian line. At present the MSP records three wavelengths of auroral emissions ...


41. Meridian Scanning Photometer Data at Zhongshan Station, Antarctica, Year 2004 [CNNADC_2004_ZhongshanStation_Antarctica_MSP_Dataset]
The Auroral Meridian Scanning Photometer is used to measure the absolute intensity of aurora brightness along the geomagnetic meridian line. At present the MSP records three wavelengths of auroral ...


42. Meridian Scanning Photometer Data at Zhongshan Station, Antarctica, Year 2005 [CNNADC_2005_Zhongshan_Station_Antarctica_MSP_Description]
The Auroral Meridian Scanning Photometer is to measure the absolute intensity of aurora brightness along the geomagnetic meridian line. At present the MSP records three wavelengths of auroral emissions ...


43. Monochromatic CCD Aurora Imager Data at Zhongshan Station, Antarctica, Year 2001 [CNNADC_2001_S_CCD_ZS]
Monochromatic CCD Aurora Imager is to monitor auroral displays at certain wavelength at nearly 180 degrees filed of view. The data is digitized images recorded on DVD-R with two copies; one for Polar ...


44. Monochromatic CCD Aurora Imager Data at Zhongshan Station, Antarctica, Year 2002 [CNNADC_2002_S_CCD_ZS]
Monochromatic CCD Aurora Imager is to monitor auroral displays at certain wavelength at nearly 180 degrees filed of view. The data is digitized images recorded on DVD-R with two copies; one for Polar ...


45. Monochromatic CCD Aurora Imager Data at Zhongshan Station, Antarctica, Year 2003 [CNNADC_S2003_S_CCD_ZS]
Monochromatic CCD Aurora Imager is to monitor auroral displays at certain wavelength at nearly 180 degrees filed of view. The data is digitized images recorded on DVD-R with two copies; one for Polar ...


46. Monochromatic CCD Aurora Imager Data at Zhongshan Station, Antarctica, Year 2005 [CNNADC_2005_Zhongshan_Station_Antarctica_CCD_IMAGER_Description]
Monochromatic CCD Aurora Imager is to monitor auroral displays at certain wavelength at nearly 180 degrees filed of view. The data is digitized images recorded on DVD-R with two copies; one for Polar ...


47. Raw data of XBT and XCTD data of CHINARE-15 (Dec. 1998-Feb. 1999) [1998-1999_15-15_S_OC_OC02_LO_O066201_000_R0_Y]
XBT and XCTD probes were droped along a section north of the Weddell Sea, Antarctica, to measure temperatures and salinities at the upper ocean (above 1000m), during the austral summer of 1998/1999.


48. Raw data of XBT and XCTD data of CHINARE-16 (Dec. 1999-Feb. 2000) [1999-2000_16-16_S_OC_OC02_LO_O066201_000_R0_Y]
XBT and XCTD probes were droped along a section north of the Weddell Sea, Antarctica, to measure temperatures and salinities at the upper ocean (above 1000m), during the austral summer of 1999/2000.


49. Sea ice temperature data at the center site of Nella Fjord, 1997, CHINARE-13 [1996-1997_13-13_S_ZS_OC05_AN_A058701_004_R0_Y]
Ice-water interface temperature data were collected in the center site (with water depth of 147.5 m) of Nella Fjord near Zhongshan Station from March to November, 1997. The data were obtained by using ...


50. Temperature and salinity from Great Wall Bay and Ardly Bay in 2005/2006 [2006TS]
Temperature and Salinity were measured with SEB CTD 19plus in Great Wall Bay (G1,G2,G3,G4,G5) and Ardly Bay (A1,A2,A3,A4,A5) in Jan. 2006.


Showing 1 through 50 of 60 Next
Click here for a static view of records.

Link to Web Site