cc: Tim Osborn , k.briffa@uea.ac.uk, masson@dsm-mail.saclay.cea.fr, hutterli@climate.unibe.ch, wanner@giub.unibe.ch, juerg@giub.unibe.ch, karin@natgeo.su.se, eystein.jansen@geo.uib.no, ddj@gfy.ku.dk, sigfus@gfy.ku.dk, guiot@cerege.fr, esper@wsl.ch, frank@wsl.ch, eavaganov@forest.akadem.ru, antti.ojala@gsf.fi, r.battarbee@geog.ucl.ac.uk, j.holmes@ucl.ac.uk, brazdil@sci.muni.cz, jerome@lgge.obs.ujf-grenoble.fr, barbante@unive.it, shishov@forest.akadem.ru date: Mon, 14 Feb 2005 16:46:25 +0100 from: Hubertus Fischer subject: Re: IMPRINT task 1.1 coming together to: petit Hi everybody, Not knowing whether this discussion is still acute I strongly support Jean-Robert's arguments. While the concentration of dust is coupled to source and transport variations, the dust size is essentially only to the latter and promises unrivaled information on long-range transport conditions. This parameter should be extensively used in the coming years as outlined in Barbara Delmonte's and Urs Ruth's work. Cheers Hubertus ----- Original Message ----- From: petit Date: Monday, February 14, 2005 2:47 pm Subject: Re: IMPRINT task 1.1 coming together > Dear Tim, > > In response to your comment nb 2 and 8 from document Task 1 > section B4 and > B8 to remove the dust studies from task 1.1 to reduce budget, I > would like > advocate for having dust project studies as part of IMPRINT. > > Recent works on dust studies from Antarctic ice cores have changed > our view > on the climate variability over the east Antarctic plateau, but > unfortunately yet not widely known. > Variability in dust size parameters during Holocene(signal/noise > ratio) is > indeed well higher and significant than other climate proxies > (e.g. stable > isotope, ...). Moreover the dust size differs from the total dust > concentration and is almost only dependant on the atmospheric > circulation > modes (Delmonte et al., 2002, 2004, and in press ). > During the last deglaciation and the Holocene period, it was shown > the size > distribution changes have been associated to the (pseudo > oscillating) > shifts of the polar vortex over East Antarctica between Dome > region and > Vostok region (Delmonte et al., 2004, and in press ). Moreover, > during > Holocene (up to 3000 BP ) significant secular to sub millennial > and secular > periodicities are present in the dust records with a dominant 200 > year > (solar?) period which is common to all records (Delmonte et al, in > press, > attached). > > Note also that such spectrum of climate sub millennial and secular > variability in Antarctica (prior 3000 BP) seems consistent with > NH variability of the last 2000 years as recently presented by > Mobek et > al, Nature, feb 10, 2005, . > GCM have been indeed used to assess the observed recent climatic > change > over Antarctica (warming Peninsula and cooling East Antarctica and > the > shift in the polar vortex) and associated due to the recent ozone > depletion > (e.g. papers from Solomon and Thompson ? in Science). > > The proposed task aims to document the 0-2000 BP period in > Antarctica from > existing ice cores and pits, with the ambition to compare with the > natural > forcings from solar variability (10Be) and volcanic input.Our task > is also > to generate dust data from pits and shallow cores covering the > instrumental period. > > Dust size studies are currently developed at Laboratory of > Glaciology > (LGGE) with collaboration with University Bicocca, Milano for > coulter > counter measurements and also University of Berne and AWI > Bremerhaven > are using laser system for flow-line analysis > > I strongly advocate for having this project part of IMPRINT which > appear > relevant to tasks1.1 task 1.2, and task 1.5. > Without this support our European community will not be able to > continue > this original and promising research. > > Sincerely yours > > Jean Robert Petit > > > > -------------------------------------------------- > Jean Robert PETIT > > LGGE-CNRS BP 96 > F-38402 St Martin d'Heres Cedex > Tel: +33 (0)4 76 82 42 44 > Fax: +33 (0)4 76 82 42 01 > > petit@lgge.obs.ujf-grenoble.fr > > http://www-lgge.obs.ujf-grenoble.fr > -------------------------------------------------- >