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39 Titles Match Your Query
Showing 1 through 39 of 39
1. 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 ...


2. All-Sky TV Camera Data at Zhongshan Station, Antarctica, Year 2002 dataset [CN_NADC_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, ...


3. 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 ...


4. 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 ...


5. 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 ...


6. 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 ...


7. 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 ...


8. 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 ...


9. 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 ...


10. 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, ...


11. 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, ...


12. 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, ...


13. 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, ...


14. 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, ...


15. Digisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica,Year 2002 [CNNADC_2002_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, ...


16. 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, ...


17. 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, ...


18. 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, ...


19. Fluxgate Magnetometer Data at Zhongshan Station in Year 2004 [CN_NADC_2004_Zhongshan_Sation_FM]
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 ...


20. 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 ...


21. 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 ...


22. 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 ...


23. Fluxgate Magnetometer Observation at Zhongshan Station in Antarctica from 1997 to 2000 [CN_NADC_FM_ZS_1997-2000]
This observation was started in Jan. 1997 at China's Zhongshan Station, Antarctica. It is designed to observe earth's magnetic field including the horizontal component in north-south direction ...


24. 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 ...


25. 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 ...


26. 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 ...


27. 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 ...


28. 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 ...


29. 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 ...


30. 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 ...


31. 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 ...


32. 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 ...


33. Monochromatic CCD Aurora Imager Data at Zhongshan Station Antarctic in 2001 [CN_NADC_CCD_ZS_2001]
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; ...


34. 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 ...


35. 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 ...


36. 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 ...


37. Monochromatic CCD Aurora Imager Data at Zhongshan Station, Antarctica, Year 2004 [CNNADC_S2004_S_CCD_ZS]
Monochromatic CCD Aurora Imager is to monitor auroral display and intensity at certain wavelength at nearly 180 degrees filed of view. The data is digitized images recorded on DVD-R with two copies; ...


38. 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 ...


39. Panchromatic all-sky TV data [1995-2000_S_ZS_GP01_LO_2001]
This is a Sino-Japan collaborative observation at Zhongshan Station, Antarctica, which commenced in March 1995 (Principal Investigators: Prof. Natsuo Sato, National Institute of Polar Research and ...


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