Data

Fabry-Perot Spectrometer Data from project 4130 - How do Antarctic space-weather disturbances propagate northward to influence ionospheric density and structure above Australia and the Southern Ocean?

Australian Antarctic Data Centre
CONDE, MARK ; ANDERSON, CALLUM ; KOSCH, MIKE ; DYSON, PETER L. ; DAVIES, THEODORE
Viewed: [[ro.stat.viewed]] Cited: [[ro.stat.cited]] Accessed: [[ro.stat.accessed]]
ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.4225/15/5ab059a125653&rft.title=Fabry-Perot Spectrometer Data from project 4130 - How do Antarctic space-weather disturbances propagate northward to influence ionospheric density and structure above Australia and the Southern Ocean?&rft.identifier=10.4225/15/5ab059a125653&rft.publisher=Australian Antarctic Data Centre&rft.description=A long-standing problem is why the mid-latitude ionosphere (eg over Australia) is sometimes enhanced during space weather storms, and sometimes depleted. While storms occur mainly at high latitudes, their effects propagate equatorward via upper atmosphere's winds, waves, electric fields, and chemical composition but we do not understand why the relative importance of these varies from storm to storm. By measuring these various drivers over Antarctica and their subsequent impacts at mid-latitude during many storms over a 5-year period we will determine the statistical importance of each driver. The spectrometers are currently based at Mawson and Davis. This record details thermospheric and mesospheric winds, temperatures, and emission intensities from the Fabry Perot Spectrometer. This project has replaced ASAC project 2699 - the data from which are held in the metadata record Fabry-Perot_Spectrometer.&rft.creator=CONDE, MARK &rft.creator=ANDERSON, CALLUM &rft.creator=KOSCH, MIKE &rft.creator=DYSON, PETER L. &rft.creator=DAVIES, THEODORE &rft.date=2013&rft.coverage=northlimit=-67.5; southlimit=-67.7; westlimit=62.8; eastLimit=62.9; projection=WGS84&rft.coverage=northlimit=-67.5; southlimit=-67.7; westlimit=62.8; eastLimit=62.9; projection=WGS84&rft.coverage=northlimit=-68.53; southlimit=-68.61; westlimit=77.92; eastLimit=78; projection=WGS84&rft.coverage=northlimit=-68.53; southlimit=-68.61; westlimit=77.92; eastLimit=78; projection=WGS84&rft_rights=This data set conforms to the CCBY Attribution License (http://creativecommons.org/licenses/by/4.0/). Please follow instructions listed in the citation reference provided at http://data.aad.gov.au/aadc/metadata/citation.cfm?entry_id=AAS_4130 when using these data.&rft_subject=climatologyMeteorologyAtmosphere&rft_subject=AIR TEMPERATURE&rft_subject=EARTH SCIENCE&rft_subject=ATMOSPHERE&rft_subject=ATMOSPHERIC TEMPERATURE&rft_subject=SURFACE TEMPERATURE&rft_subject=UPPER LEVEL WINDS&rft_subject=ATMOSPHERIC WINDS&rft_subject=MESOSPHERE&rft_subject=THERMOSPHERE&rft_subject=TEMPERATURE&rft_subject=SPECTROMETER&rft_subject=WINDS&rft_subject=FPS&rft_subject=Fabry-Perot Spectrometer&rft_subject=FPS > Fabry-Perot Spectrometer&rft_subject=FIXED OBSERVATION STATIONS&rft_subject=CONTINENT > ANTARCTICA&rft_subject=GEOGRAPHIC REGION > POLAR&rft_place=Hobart&rft.type=dataset&rft.language=English Access the data
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This data set conforms to the CCBY Attribution License (http://creativecommons.org/licenses/by/4.0/). Please follow instructions listed in the citation reference provided at http://data.aad.gov.au/aadc/metadata/citation.cfm?entry_id=AAS_4130 when using these data.

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These data are publicly available, however owing to their size are stored offline and are only available on request to the AADC. Data will be transferred via a cloud service.

Brief description

A long-standing problem is why the mid-latitude ionosphere (eg over Australia) is sometimes enhanced during space weather storms, and sometimes depleted. While storms occur mainly at high latitudes, their effects propagate equatorward via upper atmosphere's winds, waves, electric fields, and chemical composition but we do not understand why the relative importance of these varies from storm to storm. By measuring these various drivers over Antarctica and their subsequent impacts at mid-latitude during many storms over a 5-year period we will determine the statistical importance of each driver. The spectrometers are currently based at Mawson and Davis. This record details thermospheric and mesospheric winds, temperatures, and emission intensities from the Fabry Perot Spectrometer. This project has replaced ASAC project 2699 - the data from which are held in the metadata record "Fabry-Perot_Spectrometer".

Issued: 2013-07-04

Data time period: 2012-07-01 to 2013-10-31

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62.9,-67.5 62.9,-67.7 62.8,-67.7 62.8,-67.5 62.9,-67.5

62.85,-67.6

78,-68.53 78,-68.61 77.92,-68.61 77.92,-68.53 78,-68.53

77.96,-68.57

text: northlimit=-67.5; southlimit=-67.7; westlimit=62.8; eastLimit=62.9; projection=WGS84

text: northlimit=-68.53; southlimit=-68.61; westlimit=77.92; eastLimit=78; projection=WGS84

Subjects
AIR TEMPERATURE | ATMOSPHERE | ATMOSPHERIC TEMPERATURE | ATMOSPHERIC WINDS | CONTINENT > ANTARCTICA | EARTH SCIENCE | FIXED OBSERVATION STATIONS | FPS | FPS > Fabry-Perot Spectrometer | Fabry-Perot Spectrometer | GEOGRAPHIC REGION > POLAR | MESOSPHERE | SPECTROMETER | SURFACE TEMPERATURE | TEMPERATURE | THERMOSPHERE | UPPER LEVEL WINDS | WINDS | climatologyMeteorologyAtmosphere |

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AU-ANL:PEAU : http://nla.gov.au/nla.party-617536

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