Book contents
- Frontmatter
- Contents
- Preface
- Chapter 1 Introduction
- Chapter 2 Observations and instrumentation
- Chapter 3 Physical climatology
- Chapter 4 The large-scale circulation of the Antarctic atmosphere
- Chapter 5 Synoptic-scale weather systems and fronts
- Chapter 6 Mesoscale systems and processes
- Chapter 7 Climate variability and change
- Appendix A A chronological list of stations that have made multiyear meteorological observations in the Antarctic and on the sub-Antarctic islands
- Appendix B A chronological list of automatic weather stations that have been deployed in the Antarctic and on the sub-Antarctic Islands
- References
- Index
Chapter 5 - Synoptic-scale weather systems and fronts
Published online by Cambridge University Press: 02 December 2009
- Frontmatter
- Contents
- Preface
- Chapter 1 Introduction
- Chapter 2 Observations and instrumentation
- Chapter 3 Physical climatology
- Chapter 4 The large-scale circulation of the Antarctic atmosphere
- Chapter 5 Synoptic-scale weather systems and fronts
- Chapter 6 Mesoscale systems and processes
- Chapter 7 Climate variability and change
- Appendix A A chronological list of stations that have made multiyear meteorological observations in the Antarctic and on the sub-Antarctic islands
- Appendix B A chronological list of automatic weather stations that have been deployed in the Antarctic and on the sub-Antarctic Islands
- References
- Index
Summary
Introduction
Synoptic-scale weather systems, comprising the extra-tropical cyclones (depressions) and anticyclones (highs), are the main atmospheric systems found in the Antarctic coastal region and over the Southern Ocean. They typically have a horizontal length scale in the range 1000–6000 km and a lifetime of between one day and a week. Within the spectrum of atmospheric disturbances they lie between the mesoscale (less than 1000 km diameter) phenomena, such as cloud clusters, mesocyclones and squall lines, and the planetary-scale long waves that have wavelengths of many thousands of kilometres. Satellite imagery of the high southern latitudes, such as that reproduced in Figure 5.1, shows clearly the locations of the major synoptic-scale low-pressure systems through their frontal cloud bands that spiral into the centre of the systems. Such imagery is an important tool in the production of operational analyses over the Southern Hemisphere and allows the depressions to be tracked in areas sparse in data. The infra-red image shown here is of the Bellingshausen Sea on 28 April 1993 when the area was dominated by an active depression. The high, cold cloud of the front and the shower clouds in the cold air to the west of the system are the most significant features of the image.
Case studies and climatological investigations have shown that depressions form mainly on horizontal temperature gradients (baroclinic zones) in the troposphere and grow through baroclinic instability. In the Southern Hemisphere the major meridional temperature change in the troposphere occurs at the polar front separating the temperate mid-latitude air to the north and the cold polar air masses to the south.
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- Antarctic Meteorology and Climatology , pp. 185 - 266Publisher: Cambridge University PressPrint publication year: 1997
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