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Earth Observing Laboratory
Field Data Archive

DYNAMO: Darwin Radiosonde L3 Data

Summary

This is one of the upper air data sets developed for the Dynamics of the Madden-Julian Oscillation (DYNAMO) 2011-2012 project. This data set includes 737 high vertical resolution (2-sec) soundings from the Australian Bureau of Meteorology (BoM) C3 Darwin, Australia site, collected during the DYNAMO field campaign. The data were provided by ARM. There are typically four soundings per day at 00, 06, 12, and 18 UTC. The 06 and 18 UTC soundings typically contain only wind data. This L3 version of the data set has had a daytime radiation dry bias correction applied by CSU. This station used Vaisala RS92-15 radiosondes with radar-tracked winds during the DYNAMO field campaign.

Data access

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Additional information

Identifier
Data Quality final
Versions
  • 1.0 (2012-05-17)
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Related projects
Spatial Type point
Frequency 6 hourly
Language English
Categories
Platforms
Instruments
GCMD Science Keywords Expand keywords
Documentation
Related links

Temporal coverage

Begin datetime 2011-10-01 00:00:00
End datetime 2012-03-31 23:59:59

Spatial coverage


Map data from IBCSO, IBCAO, and Global Topography.

Maximum (North) Latitude: -12.42, Minimum (South) Latitude: -12.42
Minimum (West) Longitude: 130.89, Maximum (East) Longitude: 130.89

Primary point of contact information

EOL Data Support <datahelp@eol.ucar.edu>

Additional contact information

Citation

UCAR/NCAR - Earth Observing Laboratory, Australian Bureau of Meteorology, Colorado State University (CSU). 2012. DYNAMO: Darwin Radiosonde L3 Data. Version 1.0. UCAR/NCAR - Earth Observing Laboratory. https://doi.org/10.26023/KGPN-4G3F-2R07. Accessed 11 Dec 2024.

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NSF

This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.