Flight tracks and speeds of Antarctic and Atlantic seabirds: radar and optical measurements

A tracking radar and an optical range-finder, placed on a ship, were used to register the flight of eleven species of seabirds, in waters off the Antarctic Peninsula and in the Atlantic Ocean. Albatrosses under calm conditions used swell soaring, turning and twisting extensively within a width of 300-500 m laterally from the overall direction of movement. Their resulting travel speed was on average 10 m s -1 . In windy conditions the albatrosses as well as giant petrels travelled faster, with resulting speeds up to 22.5 m s -1 , by a combination of wave soaring and dynamic soaring. Shearwaters and the antarctic fulmar proceeded by flap-gliding, along tracks that were only slightly zigzag within 50-60 m from the resulting course of movement. The little shearwater flew faster, with an airspeed about 14 m s -1 , than larger-sized shearwaters and fulmars, using continuous flapping flight to a higher degree than its larger relatives. South polar skuas and Wilson’s storm-petrels were tracked on foraging flights, and flocks of imperial shags on commuting flights between feeding and breeding-roosting areas. The south polar skua was able to accelerate to airspeeds exceeding 20 m s -1 in pursuit flights after shags. Wilson’s storm-petrels showed significantly slower airspeeds in foraging flights as compared to non-foraging flights. Average airspeeds of most species fell between the minimum power and maximum range speeds estimated from aerodynamical theory. Species using gliding or flap-gliding flight showed a mean airspeed close to the gliding speed for best glide ratio. Optimal speeds in foraging flights, as expected for the south polar skuas and Wilson’s storm-petrels, are unlikely to coincide with the minimum power and maximum range speeds. Albatrosses reached the fastest resulting travel speeds when moving at angles 120°-150° from the wind (partly following winds), with strong wind forces. They predominantly travelled with the wind from their left side which, in the southern hemisphere, would lead them away from low pressure centres and towards high pressure areas.

Author(s):  
G. E. Fogg

Beginning with its dispatch of Halley on his geomagnetic cruise of 1699 to 1700, the Royal Society has played a sporadic, ad hoc, but nevertheless considerable role in the scientific investigation of the South Polar regions. In three ventures—Ross's geomagnetic survey of 1839 to 1843, the first Scott expedition of 1901 to 1904 and the British contribution to the International Geophysical Year of 1957 to 1958—it made major contributions to the planning and support of Antarctic scientific programmes. Throughout, it has given backing to polar expeditions but has been consistent in putting science before geographical discovery. It has numbered some 20 Antarctic scientists among its Fellows.


1987 ◽  
Vol 128 (1) ◽  
pp. 335-347 ◽  
Author(s):  
C. J. PENNYCUICK

Airspeeds in flapping and flap-gliding flight were measured at Foula, Shetland for three species of auks (Alcidae), three gulls (Landae), two skuas (Stercorariidae), the fulmar (Procellariidae), the gannet (Sulidae) and the shag (Phalacrocoracidae). The airspeed distributions were consistent with calculated speeds for minimum power and maximum range, except that observed speeds in the shag were unexpectedly low in relation to the calculated speeds. This is attributed to scale effects that cause the shag to have insufficient muscle power to fly much faster than its minimum power speed. The wing adaptations seen in different species are considered as deviations from a ‘procellariiform standard’, which produce separate effects on flapping and gliding speeds. Procellariiformes and the gannet flap-glide in cruising flight, but birds that swim with their wings do not, because their gliding speeds are too high in relation to their flapping speeds. Other species in the sample also do not flap-glide, but the reason is that their gliding speeds are too low in relation to their flapping speeds.


Chemosphere ◽  
1992 ◽  
Vol 24 (9) ◽  
pp. 1293-1300 ◽  
Author(s):  
Werner Reifenhäuser ◽  
Klaus G. Heumann
Keyword(s):  

1960 ◽  
Vol 54 (2) ◽  
pp. 348-371 ◽  
Author(s):  
Robert D. Hayton

The Antarctic is no longer the virtual unknown of story and legend. Though it will undoubtedly remain a frontier—as much of Alaska has remained a frontier—one consequence of the International Geophysical Year is that policy and operational affairs of the South Polar Regions have gradually become almost “orthodox,” that is, handled on a daily basis by government officials and institutions in the near-normal manner of dealing with any matter in modern bureaucracy and research.


Polar Record ◽  
1934 ◽  
Vol 1 (8) ◽  
pp. 130-142
Author(s):  
Hugh Robert Mill

The sector of the Antarctic regions between the meridians of 30° and 90° W. is still largely unknown, and offers a particularly attractive field for exploration. It was the scene of the earliest discovery of land south of the Antarctic Circle, of the earliest and also of. the latest economic exploitation of the South Polar regions and it is the only part of the Antarctic where very large areas have been seen from the air but never visited on the surface either by sea or land. It is appropriate that a concise summary of the exploration of this region should be put together, in view of the expedition now being organised by John R. Rymill with the active support of the Royal Geographical Society, the British Government, the Discovery Committee and the Polar Institute.


1996 ◽  
Vol 13 (1) ◽  
pp. 14-16 ◽  
Author(s):  
Simon P. Balm

AbstractThe Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) is a highly automated 1·7 m diameter telescope aimed at exploiting the superb submillimetre skies of the Antarctic Plateau for astronomy and aeronomy studies. It was recently installed at the Amundsen-Scott South Pole Station during the 1994/95 Austral season and is currently undergoing its first winter-over of operation. In this paper we briefly outline the capabilities of the instrument and describe some recent achievements culminating in the telescope’s first observations of the South Polar submillimetre sky.


2007 ◽  
Vol 19 (4) ◽  
pp. 507-519 ◽  
Author(s):  
Dirk van As ◽  
Michiel R. van den Broeke ◽  
Michiel M. Helsen

AbstractStrong-wind events occur 10–20 times per year at Kohnen Station, East Antarctica (75°00′S, 0°04′E, 2892 m above sea level), and are often caused by warm-core cyclones in the north-eastern Weddell Sea. An uncommon event occurred in January 2002, when blocking both in the south Atlantic Ocean and in the south Tasman Sea caused a split-up of the circumpolar vortex, and large amounts of heat and moisture were transported onto the Antarctic Plateau. During strong-wind events over the plateau the near-surface temperature can increase by tens of degrees, which is partly caused by the advection of heat, but for an important part by the destruction of the stable temperature-deficit layer by enhanced vertical mixing. The temperature rise is larger during the winter/night than during the summer/day, due to a better-developed temperature deficit. Snowdrift during the January 2002 event linearly increased surface roughness for momentum with friction velocity, for values over about 0.18 m s-1. The cloud cover during the event reduced down-welling solar radiation by 32%, and increased the albedo from about 0.86 to 0.92. Changes in longwave radiation largely cancelled the daytime changes in shortwave radiation, thus net radiation was most affected at night.


Sign in / Sign up

Export Citation Format

Share Document