Optical Properties of Deep Ice at the South Pole: Absorption The AMANDA Collaboration:

• Main Authors: P. Askebjer, S. W. Barwick, L. Bergström, A. Bouchta, S. Carius, E. Dalberg, K. Engel, B. Erl, A. Goobar, L. Gray, A. Hallgren, F. Halzen, H. Heukenkamp, P. O. Hulth, S. Hundertmark, J. Jacobsen, A. Karle V. K, I. Liubarsky, D. Lowder, T. Miller, P. Mock, R. Morse, R. Porrata, P. B. Price, A. Richards, H. Rubinstein, E. Schneider, Ch. Spiering, O. Streicher, Q. Sun, Th. Thon, S. Tilav, R. Wischnewski, Ch. Walck, G. Yodh
• Other Authors: The Pennsylvania State University CiteSeerX Archives
• Format: Text
• Language: English
• Published: 2008
• Subjects: South Pole; South pole
• Online Access: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.262.2277; http://arxiv.org/pdf/physics/9701025v1.pdf

We discuss recent measurements of the wavelength-dependent absorption coefficients in deep South Pole ice. The method uses transit time distributions of pulses from a variablefrequency laser sent between emitters and receivers embedded in the ice. At depths of 800 to 1000 m scattering is dominated by residual air bubbles, whereas absorption occurs both in ice itself and in insoluble impurities. The absorption coefficient increases approximately exponentially with wavelength in the measured interval 410 to 610 nm. At the shortest wavelength our value is about a factor 20 below previous values obtained for laboratory ice and lake ice; with increasing wavelength the discrepancy with previous measurements decreases. At ∼ 415 to ∼ 500 nm the experimental uncertainties are small enough for us to resolve an extrinsic contribution to absorption in ice: submicron dust particles contribute by an amount that increases with depth and corresponds well with the expected increase seen near the Last Glacial Maximum in Vostok and Dome C ice cores. The laser pulse method allows remote mapping of gross structure in dust concentration as a function of depth in glacial ice.