Cloud Detector measurements made at Davis Station, Antarctica

It had been shown that remote cloud detection can be performed with the use of new generation Thermopile detectors. The detection method is based on the fact that a cloudy sky will be warmer than a clear sky. An ideal cloud detection system would also need to account for the effects of relative humi...

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Other Authors: FRENCH, JOHN (hasPrincipalInvestigator), FRENCH, JOHN (processor), SYMONS, LLOYD (processor), Australian Antarctic Data Centre (publisher)
Format: Dataset
Language:unknown
Published: Australian Antarctic Data Centre
Subjects:
Online Access:https://researchdata.ands.org.au/cloud-detector-measurements-station-antarctica/699143
https://data.aad.gov.au/metadata/records/AAS_4157_Clouds
http://nla.gov.au/nla.party-617536
id ftands:oai:ands.org.au::699143
record_format openpolar
institution Open Polar
collection Research Data Australia (Australian National Data Service - ANDS)
op_collection_id ftands
language unknown
topic climatologyMeteorologyAtmosphere
CLOUDS
EARTH SCIENCE
ATMOSPHERE
CLOUD DYNAMICS
CLOUD PROPERTIES
CLOUD BASE TEMPERATURE
CLOUD FREQUENCY
Cloud sensors
Cloud detection
TNR &gt
Thermopile Net Radiometer
FIXED OBSERVATION STATIONS
GROUND STATIONS
CONTINENT &gt
ANTARCTICA
GEOGRAPHIC REGION &gt
POLAR
spellingShingle climatologyMeteorologyAtmosphere
CLOUDS
EARTH SCIENCE
ATMOSPHERE
CLOUD DYNAMICS
CLOUD PROPERTIES
CLOUD BASE TEMPERATURE
CLOUD FREQUENCY
Cloud sensors
Cloud detection
TNR &gt
Thermopile Net Radiometer
FIXED OBSERVATION STATIONS
GROUND STATIONS
CONTINENT &gt
ANTARCTICA
GEOGRAPHIC REGION &gt
POLAR
Cloud Detector measurements made at Davis Station, Antarctica
topic_facet climatologyMeteorologyAtmosphere
CLOUDS
EARTH SCIENCE
ATMOSPHERE
CLOUD DYNAMICS
CLOUD PROPERTIES
CLOUD BASE TEMPERATURE
CLOUD FREQUENCY
Cloud sensors
Cloud detection
TNR &gt
Thermopile Net Radiometer
FIXED OBSERVATION STATIONS
GROUND STATIONS
CONTINENT &gt
ANTARCTICA
GEOGRAPHIC REGION &gt
POLAR
description It had been shown that remote cloud detection can be performed with the use of new generation Thermopile detectors. The detection method is based on the fact that a cloudy sky will be warmer than a clear sky. An ideal cloud detection system would also need to account for the effects of relative humidity and barometric pressure, however good performance can still be obtained by ignoring these effects. AAD Thermopile Detector ===================== A Thermopile detector is used to remotely measure the temperature of the sky. The TPS 534 Thermopile detector chosen is fitted with a 5.5um Longpass (standard) IR filter, which allows precise remote temperature measurement of an ideal black body source. The TPS 534 Thermopile detector produces an output voltage that is positive when the temperature of the scene it is viewing is higher than the temperature of itself, and a negative output voltage when the temperature of the scene it is viewing is lower than the temperature of itself. For this reason it is necessary to compensate for the temperature of the detector. The TPS 534 Thermopile detector has an internal NTC Thermistor which can be used for temperature compensation. This Cloud Detector design implements a very simple analogue form of temperature compensation. The main drawback of an analogue temperature compensation system is that the NTC Thermistor has a very non-linear response with temperature which can only be partially corrected using a linearization resistance network. The other main drawback of an analogue temperature compensation system is that the system gains and voltage levels must be precisely adjusted by trial and error to guarantee correct operation over the desired operational temperature range. The Cloud Detector is designed for an operational temperature range of -30 degrees to +25 degrees Celsius. Operation outside of this range may cause internal signal saturation, and incorrect temperature compensation performance. The Cloud Detector optical field of view has been constrained to a 30 degrees full angle with the use of a cylindrical baffle assembly fitted directly to the Thermopile detector. The dimensions of the cylindrical baffle assembly could in theory be defined such that any field of view up to 80 degrees could be achieved. The Cloud Detector provides three plus or minus 10V output voltage signals to the data logging hardware : - Uncompensated Sensor Output Signal : Thermopile detector output signal without any analogue temperature compensation. The output voltage is proportional to the amount of cloud detected within the field of view of the instrument. - Compensated Sensor Output Signal : Thermopile detector output signal with analogue temperature compensation. The output voltage is proportional to the amount of cloud detected within the field of view of the instrument. - Temperature Output Signal : Linearised NTC Thermistor output signal used to apply analogue temperature compensation to the Thermopile detector output signal. The output voltage is proportional to the temperature of the Thermopile detector. The output voltage is uncalibrated, however the temperature verses output voltage could easily be measured. Boltwood Cloud Sensor =================== This is a commercial cloud sensor unit manufactured by diffraction limited.
author2 FRENCH, JOHN (hasPrincipalInvestigator)
FRENCH, JOHN (processor)
SYMONS, LLOYD (processor)
Australian Antarctic Data Centre (publisher)
format Dataset
title Cloud Detector measurements made at Davis Station, Antarctica
title_short Cloud Detector measurements made at Davis Station, Antarctica
title_full Cloud Detector measurements made at Davis Station, Antarctica
title_fullStr Cloud Detector measurements made at Davis Station, Antarctica
title_full_unstemmed Cloud Detector measurements made at Davis Station, Antarctica
title_sort cloud detector measurements made at davis station, antarctica
publisher Australian Antarctic Data Centre
url https://researchdata.ands.org.au/cloud-detector-measurements-station-antarctica/699143
https://data.aad.gov.au/metadata/records/AAS_4157_Clouds
http://nla.gov.au/nla.party-617536
op_coverage Spatial: northlimit=-68.57612; southlimit=-68.57612; westlimit=77.972; eastLimit=77.972; projection=WGS84
Temporal: From 2002-11-01
long_lat ENVELOPE(-67.083,-67.083,-68.200,-68.200)
ENVELOPE(77.968,77.968,-68.576,-68.576)
ENVELOPE(77.968,77.968,-68.576,-68.576)
ENVELOPE(77.972,77.972,-68.57612,-68.57612)
geographic Baffle
Davis Station
Davis-Station
geographic_facet Baffle
Davis Station
Davis-Station
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source Australian Antarctic Data Centre
op_relation https://researchdata.ands.org.au/cloud-detector-measurements-station-antarctica/699143
7ec09527-1104-4b63-a5b9-0ad8210dd15d
AAS_4157_Clouds
https://data.aad.gov.au/metadata/records/AAS_4157_Clouds
http://nla.gov.au/nla.party-617536
_version_ 1766245802727964672
spelling ftands:oai:ands.org.au::699143 2023-05-15T13:46:57+02:00 Cloud Detector measurements made at Davis Station, Antarctica FRENCH, JOHN (hasPrincipalInvestigator) FRENCH, JOHN (processor) SYMONS, LLOYD (processor) Australian Antarctic Data Centre (publisher) Spatial: northlimit=-68.57612; southlimit=-68.57612; westlimit=77.972; eastLimit=77.972; projection=WGS84 Temporal: From 2002-11-01 https://researchdata.ands.org.au/cloud-detector-measurements-station-antarctica/699143 https://data.aad.gov.au/metadata/records/AAS_4157_Clouds http://nla.gov.au/nla.party-617536 unknown Australian Antarctic Data Centre https://researchdata.ands.org.au/cloud-detector-measurements-station-antarctica/699143 7ec09527-1104-4b63-a5b9-0ad8210dd15d AAS_4157_Clouds https://data.aad.gov.au/metadata/records/AAS_4157_Clouds http://nla.gov.au/nla.party-617536 Australian Antarctic Data Centre climatologyMeteorologyAtmosphere CLOUDS EARTH SCIENCE ATMOSPHERE CLOUD DYNAMICS CLOUD PROPERTIES CLOUD BASE TEMPERATURE CLOUD FREQUENCY Cloud sensors Cloud detection TNR &gt Thermopile Net Radiometer FIXED OBSERVATION STATIONS GROUND STATIONS CONTINENT &gt ANTARCTICA GEOGRAPHIC REGION &gt POLAR dataset ftands 2020-01-05T21:15:47Z It had been shown that remote cloud detection can be performed with the use of new generation Thermopile detectors. The detection method is based on the fact that a cloudy sky will be warmer than a clear sky. An ideal cloud detection system would also need to account for the effects of relative humidity and barometric pressure, however good performance can still be obtained by ignoring these effects. AAD Thermopile Detector ===================== A Thermopile detector is used to remotely measure the temperature of the sky. The TPS 534 Thermopile detector chosen is fitted with a 5.5um Longpass (standard) IR filter, which allows precise remote temperature measurement of an ideal black body source. The TPS 534 Thermopile detector produces an output voltage that is positive when the temperature of the scene it is viewing is higher than the temperature of itself, and a negative output voltage when the temperature of the scene it is viewing is lower than the temperature of itself. For this reason it is necessary to compensate for the temperature of the detector. The TPS 534 Thermopile detector has an internal NTC Thermistor which can be used for temperature compensation. This Cloud Detector design implements a very simple analogue form of temperature compensation. The main drawback of an analogue temperature compensation system is that the NTC Thermistor has a very non-linear response with temperature which can only be partially corrected using a linearization resistance network. The other main drawback of an analogue temperature compensation system is that the system gains and voltage levels must be precisely adjusted by trial and error to guarantee correct operation over the desired operational temperature range. The Cloud Detector is designed for an operational temperature range of -30 degrees to +25 degrees Celsius. Operation outside of this range may cause internal signal saturation, and incorrect temperature compensation performance. The Cloud Detector optical field of view has been constrained to a 30 degrees full angle with the use of a cylindrical baffle assembly fitted directly to the Thermopile detector. The dimensions of the cylindrical baffle assembly could in theory be defined such that any field of view up to 80 degrees could be achieved. The Cloud Detector provides three plus or minus 10V output voltage signals to the data logging hardware : - Uncompensated Sensor Output Signal : Thermopile detector output signal without any analogue temperature compensation. The output voltage is proportional to the amount of cloud detected within the field of view of the instrument. - Compensated Sensor Output Signal : Thermopile detector output signal with analogue temperature compensation. The output voltage is proportional to the amount of cloud detected within the field of view of the instrument. - Temperature Output Signal : Linearised NTC Thermistor output signal used to apply analogue temperature compensation to the Thermopile detector output signal. The output voltage is proportional to the temperature of the Thermopile detector. The output voltage is uncalibrated, however the temperature verses output voltage could easily be measured. Boltwood Cloud Sensor =================== This is a commercial cloud sensor unit manufactured by diffraction limited. Dataset Antarc* Antarctica Research Data Australia (Australian National Data Service - ANDS) Baffle ENVELOPE(-67.083,-67.083,-68.200,-68.200) Davis Station ENVELOPE(77.968,77.968,-68.576,-68.576) Davis-Station ENVELOPE(77.968,77.968,-68.576,-68.576) ENVELOPE(77.972,77.972,-68.57612,-68.57612)