J. D. Shanklin
British Antarctic Survey
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Featured researches published by J. D. Shanklin.
Polar Record | 2014
John Turner; Nicholas E. Barrand; Thomas J. Bracegirdle; Peter Convey; Dominic A. Hodgson; Martin J. Jarvis; Adrian Jenkins; Gareth J. Marshall; Michael P. Meredith; Howard K. Roscoe; J. D. Shanklin; John Anthony French; Hugues Goosse; Mauro Guglielmin; Julian Gutt; Stan Jacobs; M. C. Kennicutt; Valérie Masson-Delmotte; Paul Andrew Mayewski; Francisco Navarro; Sharon A. Robinson; Theodore A. Scambos; M. Sparrow; Colin Summerhayes; Kevin G. Speer; A. Klepikov
We present an update of the ‘key points’ from the Antarctic Climate Change and the Environment (ACCE) report that was published by the Scientific Committee on Antarctic Research (SCAR) in 2009. We summarise subsequent advances in knowledge concerning how the climates of the Antarctic and Southern Ocean have changed in the past, how they might change in the future, and examine the associated impacts on the marine and terrestrial biota. We also incorporate relevant material presented by SCAR to the Antarctic Treaty Consultative Meetings, and make use of emerging results that will form part of the Intergovernmental Panel on Climate Change (IPCC) Fifth Assessment Report
Journal of the Atmospheric Sciences | 2005
Howard K. Roscoe; J. D. Shanklin; Steve Colwell
In late September 2002, the Antarctic ozone hole was seen to split into two parts, resulting in large increases in ozone at some stations and the potential for significant modification of chlorofluorocarbon (CFC)-induced ozone loss. The phenomenon was dynamical (a split vortex), causing large increases in stratospheric temperature above stations normally within the vortex. Temperatures at Halley, Antarctica, at 30 hPa increased by over 60 K, and temperatures at South Pole at 100 hPa increased by over 25 K. It is important to know if this has happened before, since if it happens in the future, it would significantly alter the total hemispheric ozone loss due to chlorine from CFCs, particularly if it happens in August or September. Temperatures in winter and spring measured at Halley or the South Pole since 1957 and 1961, respectively, show no other comparable increases until the final warming in late spring, except for two dates in the 1980s at Halley when meteorological analyses show no vortex split. There are very few periods of measurements missing at both Halley and the South Pole, and analyses in those few periods show no vortex split. Measurements in August and September at sites normally near the edge of the vortex show very few suspicious dates, and analyses of those few suspicious dates again show no vortex split. It is concluded that the vortex has probably not split before the final warming since Antarctic records began in the late 1950s, and almost certainly not in August or September.
Archive | 2009
Byron J. Adams; Rob Arthern; Angus Atkinson; Carlo Barbante; Roberto Bargagli; Dana M. Bergstrom; Nancy A. N. Bertler; Robert Bindschadler; James Bockheim; Claude Boutron; David Bromwich; Steve Chown; Josifino Comiso; Peter Convey; Alison Cook; Guido di Prisco; Eberhard Fahrbach; Jim Fastook; Jaume Forcada; Josep-Maria Gili; Mauro Gugliemin; Julian Gutt; Hartmut Hellmer; Françoise Hennion; Karen Heywood; Dominic A. Hodgson; David Holland; Sungmin Hong; Ad H L Huiskes; Enrique Isla
The instrumental period began with the first voyages to the Southern Ocean during the Seventeenth and Eighteenth centuries when scientists such as Edmund Halley made observations of quantities such as geomagnetism. During the early voyages information was collected on the meteorological conditions across the Southern Ocean, ocean conditions, the sea ice extent and the terrestrial and marine biology. The continent itself was discovered in 1820, although the collection of data was sporadic through the remainder of the Nineteenth Century and it was not possible to venture into the inhospitable interior of Antarctica. At the start of the Twentieth Century stations were first operated year-round and this really began the period of organised scientific investigation in the Antarctic. Most of these stations were not operated for long periods, which is a handicap when trying to investigate climate change over the last century.
Atmospheric Chemistry and Physics | 2013
Jayanarayanan Kuttippurath; Franck Lefèvre; Jean-Pierre Pommereau; Howard K. Roscoe; Florence Goutail; Andrea Pazmino; J. D. Shanklin
Atmospheric Chemistry and Physics | 2005
R. E. Hibbins; J. D. Shanklin; P. J. Espy; Martin J. Jarvis; Dennis M. Riggin; David C. Fritts; F.-J. Lübken
Quarterly Journal of the Royal Meteorological Society | 2003
Howard K. Roscoe; Steve Colwell; J. D. Shanklin
Archive | 2003
J.-C. Lambert; J. Granville; M. Allaart; Thomas Blumenstock; T. Coosemans; M. De Mazière; Udo Friess; M. Gil; Florence Goutail; Dmitry V. Ionov; I. Kostadinov; E. Kyrö; A. Petritoli; Ankie Piters; Andreas Richter; Howard K. Roscoe; H. Schets; J. D. Shanklin; Vincent T. Soebijanta; T. Suortti; M. Van Roozendael; C. Varotsos; T. Wagner
Advances in Space Research | 2005
Howard K. Roscoe; Steve Colwell; J. D. Shanklin; J.A. Karhu; Petteri Taalas; M. Gil; M. Yela; S. Rodriguez; C. Rafanelli; H. Cazeneuve; C.A. Villanueva; M. Ginsburg; S.B. Diaz; R.L. de Zafra; Giovanni Muscari; G. Redaelli; R. Dragani
Archive | 2004
J.-C. Lambert; M Allaart; S. B. Andersen; Thomas Blumenstock; Greg Bodeker; Ellen Brinksma; C. Cambridge; Martine De Mazière; Philippe Demoulin; P. Gerard; M. Gil; Florence Goutail; J. Granville; Dmitry V. Ionov; E. Kyrö; N. Navarro-Comas; A. Piters; Jean-Pierre Pommereau; Andreas Richter; Howard K. Roscoe; H. Schets; J. D. Shanklin; T. Suortti; Ralf Sussmann; Michel Van Roozendael; C. Varotsos; T. Wagner; S. W. Wood; Margarita Yela
Atmospheric Chemistry and Physics | 2012
Jayanarayanan Kuttippurath; Franck Lefèvre; J.-P. Pommereau; Howard K. Roscoe; Florence Goutail; Andrea Pazmino; J. D. Shanklin