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Scanning Photometer Data in Zhongshan Station, Antarctica

Listed in NASA Earthdata CMR

Description

The Meridian Scanning Photometer installed at Zhongshan Station is one of the Polar Research Institute of China (PRIC) and the National Institute of Polar Research (NIPR) of Japan cooperative projects, which observes aurora variations in three wavelengths (427.8nm, 557.7nm and 630nm) along the invariant meridian; its scanning range extends almost from horizon to horizon. The observation was started in March 1995. However, it was interrupted during the period of July 1995 through Feb. 1997.

The data is only valid for dark time. In other words, there is no valid data during the middle of October to the beginning of March every year.

Links

Topics

Provenance · 1 source records, 10 field assertions
SourceKeyLast seenRaw
NASA Earthdata CMRC1214608750-SCIOPS10 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[instrument].gcmd_instrument:photometerssource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[measured_variable].gcmd:earth-science/spectral-engineering/visible-wavelengths/sensor-countssource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/ionosphere-magnetosphere-dynamics/auroraesource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[platform].gcmd_platform:not-providedsource · NASA CMRconnector:nasa_cmr@1.0.0
descriptionsource · NASA CMRconnector:nasa_cmr@1.0.0/umm/Abstract
spatialsource · NASA CMRconnector:nasa_cmr@1.0.0/umm/SpatialExtent
temporalsource · NASA CMRconnector:nasa_cmr@1.0.0/umm/TemporalExtents
titlesource · NASA CMRconnector:nasa_cmr@1.0.0/umm/EntryTitle
version_labelsource · NASA CMRconnector:nasa_cmr@1.0.0