In this paper an examination of all available data on the hydrological
characteristics of the Tasman Sea, prior to and including the year 1954, has permitted
the identification and naming of eight surface water masses. Certain of
their properties and general features of their season and region of occurrence and
method of formation are summarized.
Although little quantitative data are available some general features of the
circulation of these water masses in the Tasman Sea are deduced from a study of
their seasonal occurrence in relation to source regions.
The Coral Sea water mass (chlorinity 19.60-19.70‰, temperature 20-26� C)
flows from a source region in the north-west Coral Sea along the western side of
the Tasman Sea and reaches maximum velocity off Sydney in October-December.
The South Equatorial (chlorinity 19.50-19.60‰, temperature 24-26� C) also flows
south along the western side of the Tasman Sea but reaches maximum velocity
between February and March. These two water masses constitute the East
Australian current.
The Sub-Antarctic (chlorinity 19.15-19.30‰, temperature 10-14°C) is
found at the surface in the south-eastern Tasman Sea between July and September.
The Central Tasman (chlorinity 19.65-19.75‰, temperature 15-20‰C) flows to the
west from its region of formation and generally flows north along the southern
New South Wales coast in late winter. The South-west Tasman (chlorinity 19.50-
19.60‰, temperature 12-15°C) flows to the east in latitude 38�S. and curves south
in a clockwise gyral off eastern Tasmania between October and December. The Xorth
Bass Strait (chlorinity 19.66-19.75‰ temperature 12-17�C) flows from South
Australia to the eastern approaches of Bass Strait. The East Central New Zealand
(chlorinity 19.10-19.30‰, temperature 15-20°C) flows west through Cook Strait into
the Tasman Sea in midsummer. The East and West Tasmanian (chlorinity 19.40-
19.50‰ temperature 10-14°C) form in midwinter in the southern part of Bass
Strait and flow along the east and west coasts in the spring.