Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice

The depth-dependence of bubble concentration at pressures above the transition to the air hydrate phase and the optical scattering length due to bubbles in deep ice at the South Pole are modeled using diffusion-growth data from the laboratory, taking into account the dependence of age and temperatur...

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Bibliographic Details
Main Author: Price, P B
Language:English
Published: 1995
Subjects:
Online Access:http://cds.cern.ch/record/275350
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spelling ftcern:oai:cds.cern.ch:275350 2023-05-15T14:01:57+02:00 Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice Price, P B 1995-01-19 http://cds.cern.ch/record/275350 eng eng http://cds.cern.ch/record/275350 astro-ph/9501073 oai:cds.cern.ch:275350 Astrophysics and Astronomy 1995 ftcern 2018-07-28T02:33:08Z The depth-dependence of bubble concentration at pressures above the transition to the air hydrate phase and the optical scattering length due to bubbles in deep ice at the South Pole are modeled using diffusion-growth data from the laboratory, taking into account the dependence of age and temperature on depth in the ice. The model fits the available data on bubbles in cores from Vostok and Byrd and on scattering length in deep ice at the South Pole. It explains why bubbles and air hydrate crystals co-exist in deep ice over a range of depths as great as 800 m and predicts that at depths below \rm \sim 1400 m the AMANDA neutrino observatory at the South Pole will operate unimpaired by light scattering from bubbles. Other/Unknown Material Antarc* Antarctic South pole South pole CERN Document Server (CDS) Antarctic Byrd South Pole
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Price, P B
Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice
topic_facet Astrophysics and Astronomy
description The depth-dependence of bubble concentration at pressures above the transition to the air hydrate phase and the optical scattering length due to bubbles in deep ice at the South Pole are modeled using diffusion-growth data from the laboratory, taking into account the dependence of age and temperature on depth in the ice. The model fits the available data on bubbles in cores from Vostok and Byrd and on scattering length in deep ice at the South Pole. It explains why bubbles and air hydrate crystals co-exist in deep ice over a range of depths as great as 800 m and predicts that at depths below \rm \sim 1400 m the AMANDA neutrino observatory at the South Pole will operate unimpaired by light scattering from bubbles.
author Price, P B
author_facet Price, P B
author_sort Price, P B
title Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice
title_short Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice
title_full Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice
title_fullStr Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice
title_full_unstemmed Kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice
title_sort kinetics of conversion of air bubbles to air-hydrate crystals in antarctic ice
publishDate 1995
url http://cds.cern.ch/record/275350
geographic Antarctic
Byrd
South Pole
geographic_facet Antarctic
Byrd
South Pole
genre Antarc*
Antarctic
South pole
South pole
genre_facet Antarc*
Antarctic
South pole
South pole
op_relation http://cds.cern.ch/record/275350
astro-ph/9501073
oai:cds.cern.ch:275350
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