Constarium
← Search

Data · collection · 2011

Upper atmosphere winds, temperatures, and emission intensities

Listed in NASA Earthdata CMR

The spectrometers are currently based at Mawson and Davis.

Description

This record details thermospheric and mesospheric winds, temperatures, and emission intensities from the Fabry Perot Spectrometer. See the publications database for a list of references associated with the project - ASAC projects 514 and 2699.

Project objectives: The principle aim of the project is to detect upwellings in thermospheric wind, characterise their properties at different levels in the thermosphere (~100 km and ~200 km altitude); and determine their impact on the mesosphere and ionosphere. The project will also: (i) systematically study the dynamics and thermodynamics of the Antarctic thermosphere and mesosphere by observing the winds and temperatures in these regions; (ii) identify the propagation of atmospheric gravity waves (AGWs) in the thermosphere and mesosphere; (iii) investigate the sources of AGWs in the thermosphere and their impact on the ionosphere; (iv) monitor the long term behaviour of the thermosphere and mesosphere for changes possibly related to global change; Taken from the 2008-2009 Progress Report: Public summary of the season progress: The Davis Fabry-Perot Spectrometer, installed in 2003-04, continues to operate successfully and autonomously.

Read the rest (3 more)

Yearly modifications have improved the quality of observations and the instrument's reliability. Data is downloaded periodically to La Trobe University to monitor performance and new campaign modes are uploaded from La Trobe. The successful 2008 operations provided new observations on the behaviour of winds and temperatures in the thermosphere, a region of the atmosphere drastically affected by space weather.

Current research concentrates on investigating the high-latitude sources of atmospheric gravity waves, and processes that control the more regular, daily, seasonal and annual variations in wind and temperature. Taken from the 2009-2010 Progress Report: Public summary of the season progress: There is a high degree of symmetry in the charged particle energy inputs to the northern and southern hemisphere that drive auroral processes.

Results from this project combined with simultaneous observations in Scandinavia have shown for the first time that winds at heights of about 250 km in the thermospheric region of the neutral atmosphere respond rapidly to the motions in the auroral ionosphere and also have a high degree of symmetry.

Links

Get the data

Catalogue records · 2

Topics

Inferred from text
Atmospheric sciences 73%
Provenance · 1 source records, 14 field assertions
SourceKeyLast seenRaw
NASA Earthdata CMRC1214308564-AU_AADC13 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[field].anzsrc:group:3701enrichment · NASA CMRtaxonomy-embedding@1.1.0title+keywords+description (73%)
concepts[instrument].gcmd_instrument:fpssource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[instrument].gcmd_instrument:spectrometerssource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[measured_variable].gcmd:earth-science/atmosphere/atmospheric-temperature/surface-temperature/air-temperaturesource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[measured_variable].gcmd:earth-science/atmosphere/atmospheric-winds/upper-level-windssource · NASA CMRconnector:nasa_cmr@1.0.0
concepts[platform].gcmd_platform:fixed-observation-stationssource · NASA CMRconnector:nasa_cmr@1.0.0
descriptionsource · NASA CMRconnector:nasa_cmr@1.0.0/umm/Abstract
license_textsource · NASA CMRconnector:nasa_cmr@1.0.0
publication_datesource · NASA CMRconnector:nasa_cmr@1.0.0
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