| 25 Titles Match Your Query |
Showing 1 through 25 of 25
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1.
Ozone data at the Zhongshan station, Antarctica during the 21st CHINARE in 2004 [CNNADC_2004_Zhongshan_Station_Location_SensorName_Description]
Data recorded by ozone spectroapparatus in ZhongShan station.Those data include ozone and S02 data by BREWER exploration, which happened at noon time. At that time the radiation between the scope ...
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2.
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 ...
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3.
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, ...
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4.
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, ...
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5.
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, ...
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6.
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 ...
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7.
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 ...
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8.
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 ...
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9.
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; ...
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10.
Yearly characteristics on the weather and climate of the Great Wall Station and Zhongshan Station, Antarctica from 1985 to 2000 [CNNADC_1985-2000_GWZS_station_Climate_Index]
The monthly mean of surface meteorological data at Geat Wall Station and Zhongshan Station,Antarctic.
-Atmospheric pressure at Station level( hPa )
-Air temperature of 1.5 m above the ...
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11.
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 ...
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12.
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 ...
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13.
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 ...
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14.
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 ...
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15.
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 ...
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16.
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 ...
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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, ...
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18.
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 ...
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19.
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 ...
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20.
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 ...
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21.
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 ...
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22.
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 ...
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23.
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, ...
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24.
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, ...
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25.
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 ...
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Showing 1 through 25 of 25
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