Chemical and isotopic snow variability in East Antarctica along the 2001/02 ITASE traverse

被引:35
作者
Becagli, S
Proposito, M
Benassai, S
Flora, O
Genoni, L
Gragnani, R
Largiuni, O
Pili, SL
Severi, M
Stenni, B
Traversi, R
Udisti, R
Frezzott, M
机构
[1] Univ Florence, Dept Chem, I-50019 Sesto Fiorenti, Italy
[2] Museo Nazl Antartide, I-53100 Siena, Italy
[3] Univ Trieste, Dept Geol Environm & Marine, I-34127 Trieste, Italy
[4] ENEA, Ctr Ric, I-00100 Rome, Italy
[5] Univ Cagliari, Dept Earth Sci, I-09127 Cagliari, Italy
来源
ANNALS OF GLACIOLOGY, VOL 39, 2004 | 2004年 / 39卷
关键词
D O I
10.3189/172756404781814636
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
As part of the International Trans-Antarctic Scientific Expedition (ITASE) project, a traverse was carried out from November 2001 to January 2002 through Terre Adelie, George V Land, Oates Land and northern Victoria Land, for a total length of about 1875 km. The research goal is to determine the latitudinal and longitudinal variability of physical, chemical and isotopic parameters along three transects: one west-east transect (WE), following the 2150 m contour line (about 400 km inland of the Adelie, George V and Oates coasts), and two north-south transects (inland Terre Adelie and Oates Coast-Talos Dome-Victoria Land). The intersection between the WE and Oates Coast-Victoria Land transects is in the Talos Dome area. Along the traverse, eight 2 m deep snow pits were dug and sampled with a 2.5 cm depth resolution. For spatial variability, I m deep integrated samples were collected every 5 km (363 sampling sites). In the snow-pit stratigraphy, pronounced annual cycles, with summer maxima, were observed for nssSO(4)(2-), MSA, NO3- and H2O2. The seasonality of these chemical trace species was used in combination with stable-isotope stratigraphy to derive reliable and temporally representative snow-accumulation rates. The study of chemical, isotopic and accumulation-rate variability allowed the identification of a distribution pattern which is controlled not only by altitude and distance from the sea, but also by the complex circulation of air masses in the study area. In particular, although the Talos Dome area is almost equidistant from the Southern Ocean and the Ross Sea, local atmospheric circulation is such that the area is strongly affected only by the Ross Sea. Moreover, we observed a decrease in concentration of aerosol components in the central portion of the WE transect and in the southern portion of the Talos Dome transect; this decrease was linked to the higher stability of atmospheric pressure due to the channelling of katabatic winds.
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收藏
页码:473 / 482
页数:10
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