The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia)

Motivated by the record-breaking heatwaves of early 2017, the synoptic structure and evolution of summer (December–February) heatwaves in the Sydney area is investigated through composite and trajectory analyses. In the upper troposphere, the main features of the composite structure are an isolated...

Full description

Bibliographic Details
Main Authors: Parker, Tess, Quinting, Julian, Reeder, Michael
Format: Text
Language:English
Published: Bureau of Meteorology 2020
Subjects:
Online Access:https://dx.doi.org/10.5445/ir/1000120169
https://publikationen.bibliothek.kit.edu/1000120169
id ftdatacite:10.5445/ir/1000120169
record_format openpolar
spelling ftdatacite:10.5445/ir/1000120169 2023-05-15T18:25:58+02:00 The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia) Parker, Tess Quinting, Julian Reeder, Michael 2020 PDF https://dx.doi.org/10.5445/ir/1000120169 https://publikationen.bibliothek.kit.edu/1000120169 en eng Bureau of Meteorology Creative Commons Namensnennung – Nicht kommerziell – Keine Bearbeitungen 4.0 International Open Access info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-nd/4.0/deed.de CC-BY-NC-ND Text article-journal Journal Article ScholarlyArticle 2020 ftdatacite https://doi.org/10.5445/ir/1000120169 2021-11-05T12:55:41Z Motivated by the record-breaking heatwaves of early 2017, the synoptic structure and evolution of summer (December–February) heatwaves in the Sydney area is investigated through composite and trajectory analyses. In the upper troposphere, the main features of the composite structure are an isolated upper-tropospheric anticyclonic potential vorticity (PV) anomaly to the south-east of Australia and cyclonic anomalies to the east and south. Back trajectories starting from within the upper-tropospheric anticyclonic PV anomaly on the first day of the heatwave fall into two groups: those that are diabatically cooled in the final 72 h and those that are diabatically heated. Those that are cooled come predominantly from the upstreammiddle troposphere over the Indian Ocean. The change in the potential temperature of these parcels is less than 3K, and so their motion is effectively adiabatic. In contrast, those parcels that are heated in the final 72 h are drawn predominantly from the lower half of the troposphere over the south-western part of the continent. As they ascended, their potential temperature increases by 10K in the mean due to latent heating. At low-levels, the main features of the composite are an anticyclone centred in the Tasman Sea, a broad low over the Southern Ocean and associated anomalous warmnorthwesterlies over the Sydney area. Five days prior to the heatwave, air parcels that become part of the near surface air mass are located predominantly offshore to the east and south of the continent. The anomalously high surface temperatures can be explained by adiabatic compression and surface sensible heating. For the next 48 h, the air parcels subside and their potential temperature changes little, whereas their temperature increases by around 15Kthrough adiabatic compression. In the final 72 h, as the parcels approach the surface and are entrained into the boundary layer, the potential temperature and temperature both increase by 5K, presumably through surface sensible heating. The record-breaking heatwaves of January and February 2017 are found to be very representative of previous heatwaves in the Sydney area, and in the mean they are synoptically very similar to heatwaves in Victoria, although dynamically there are differences. Text Southern Ocean DataCite Metadata Store (German National Library of Science and Technology) Southern Ocean Indian
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language English
description Motivated by the record-breaking heatwaves of early 2017, the synoptic structure and evolution of summer (December–February) heatwaves in the Sydney area is investigated through composite and trajectory analyses. In the upper troposphere, the main features of the composite structure are an isolated upper-tropospheric anticyclonic potential vorticity (PV) anomaly to the south-east of Australia and cyclonic anomalies to the east and south. Back trajectories starting from within the upper-tropospheric anticyclonic PV anomaly on the first day of the heatwave fall into two groups: those that are diabatically cooled in the final 72 h and those that are diabatically heated. Those that are cooled come predominantly from the upstreammiddle troposphere over the Indian Ocean. The change in the potential temperature of these parcels is less than 3K, and so their motion is effectively adiabatic. In contrast, those parcels that are heated in the final 72 h are drawn predominantly from the lower half of the troposphere over the south-western part of the continent. As they ascended, their potential temperature increases by 10K in the mean due to latent heating. At low-levels, the main features of the composite are an anticyclone centred in the Tasman Sea, a broad low over the Southern Ocean and associated anomalous warmnorthwesterlies over the Sydney area. Five days prior to the heatwave, air parcels that become part of the near surface air mass are located predominantly offshore to the east and south of the continent. The anomalously high surface temperatures can be explained by adiabatic compression and surface sensible heating. For the next 48 h, the air parcels subside and their potential temperature changes little, whereas their temperature increases by around 15Kthrough adiabatic compression. In the final 72 h, as the parcels approach the surface and are entrained into the boundary layer, the potential temperature and temperature both increase by 5K, presumably through surface sensible heating. The record-breaking heatwaves of January and February 2017 are found to be very representative of previous heatwaves in the Sydney area, and in the mean they are synoptically very similar to heatwaves in Victoria, although dynamically there are differences.
format Text
author Parker, Tess
Quinting, Julian
Reeder, Michael
spellingShingle Parker, Tess
Quinting, Julian
Reeder, Michael
The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia)
author_facet Parker, Tess
Quinting, Julian
Reeder, Michael
author_sort Parker, Tess
title The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia)
title_short The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia)
title_full The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia)
title_fullStr The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia)
title_full_unstemmed The synoptic-dynamics of summertime heatwaves in the Sydney area (Australia)
title_sort synoptic-dynamics of summertime heatwaves in the sydney area (australia)
publisher Bureau of Meteorology
publishDate 2020
url https://dx.doi.org/10.5445/ir/1000120169
https://publikationen.bibliothek.kit.edu/1000120169
geographic Southern Ocean
Indian
geographic_facet Southern Ocean
Indian
genre Southern Ocean
genre_facet Southern Ocean
op_rights Creative Commons Namensnennung – Nicht kommerziell – Keine Bearbeitungen 4.0 International
Open Access
info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-nd/4.0/deed.de
op_rightsnorm CC-BY-NC-ND
op_doi https://doi.org/10.5445/ir/1000120169
_version_ 1766207728570597376