author_facet Arndt, Stefanie
Willmes, Sascha
Dierking, Wolfgang
Nicolaus, Marcel
Arndt, Stefanie
Willmes, Sascha
Dierking, Wolfgang
Nicolaus, Marcel
author Arndt, Stefanie
Willmes, Sascha
Dierking, Wolfgang
Nicolaus, Marcel
spellingShingle Arndt, Stefanie
Willmes, Sascha
Dierking, Wolfgang
Nicolaus, Marcel
Journal of Geophysical Research: Oceans
Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
Earth and Planetary Sciences (miscellaneous)
Space and Planetary Science
Geochemistry and Petrology
Geophysics
Oceanography
author_sort arndt, stefanie
spelling Arndt, Stefanie Willmes, Sascha Dierking, Wolfgang Nicolaus, Marcel 2169-9275 2169-9291 American Geophysical Union (AGU) Earth and Planetary Sciences (miscellaneous) Space and Planetary Science Geochemistry and Petrology Geophysics Oceanography http://dx.doi.org/10.1002/2015jc011504 <jats:title>Abstract</jats:title><jats:p>An improved understanding of the temporal variability and the spatial distribution of snowmelt on Antarctic sea ice is crucial to better quantify atmosphere‐ice‐ocean interactions, in particular sea‐ice mass and energy budgets. It is therefore important to understand the mechanisms that drive snowmelt, both at different times of the year and in different regions around Antarctica. In this study, we combine diurnal brightness temperature differences (dT<jats:sub>B</jats:sub>(37 GHz)) and ratios (T<jats:sub>B</jats:sub>(19 GHz)/T<jats:sub>B</jats:sub>(37 GHz)) to detect and classify snowmelt processes. We distinguish temporary snowmelt from continuous snowmelt to characterize dominant melt patterns for different Antarctic sea‐ice regions from 1988/1989 to 2014/2015. Our results indicate four characteristic melt types. On average, 38.9 ± 6.0% of all detected melt events are diurnal freeze‐thaw cycles in the surface snow layer, characteristic of temporary melt (Type A). Less than 2% reveal immediate continuous snowmelt throughout the snowpack, i.e., strong melt over a period of several days (Type B). In 11.7 ± 4.0%, Type A and B take place consecutively (Type C), and for 47.8 ± 6.8% no surface melt is observed at all (Type D). Continuous snowmelt is primarily observed in the outflow of the Weddell Gyre and in the northern Ross Sea, usually 17 days after the onset of temporary melt. Comparisons with Snow Buoy data suggest that also the onset of continuous snowmelt does not translate into changes in snow depth for a longer period but might rather affect the internal stratigraphy and density structure of the snowpack. Considering the entire data set, the timing of snowmelt processes does not show significant temporal trends.</jats:p> Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations Journal of Geophysical Research: Oceans
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title Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_unstemmed Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_full Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_fullStr Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_full_unstemmed Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_short Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_sort timing and regional patterns of snowmelt on antarctic sea ice from passive microwave satellite observations
topic Earth and Planetary Sciences (miscellaneous)
Space and Planetary Science
Geochemistry and Petrology
Geophysics
Oceanography
url http://dx.doi.org/10.1002/2015jc011504
publishDate 2016
physical 5916-5930
description <jats:title>Abstract</jats:title><jats:p>An improved understanding of the temporal variability and the spatial distribution of snowmelt on Antarctic sea ice is crucial to better quantify atmosphere‐ice‐ocean interactions, in particular sea‐ice mass and energy budgets. It is therefore important to understand the mechanisms that drive snowmelt, both at different times of the year and in different regions around Antarctica. In this study, we combine diurnal brightness temperature differences (dT<jats:sub>B</jats:sub>(37 GHz)) and ratios (T<jats:sub>B</jats:sub>(19 GHz)/T<jats:sub>B</jats:sub>(37 GHz)) to detect and classify snowmelt processes. We distinguish temporary snowmelt from continuous snowmelt to characterize dominant melt patterns for different Antarctic sea‐ice regions from 1988/1989 to 2014/2015. Our results indicate four characteristic melt types. On average, 38.9 ± 6.0% of all detected melt events are diurnal freeze‐thaw cycles in the surface snow layer, characteristic of temporary melt (Type A). Less than 2% reveal immediate continuous snowmelt throughout the snowpack, i.e., strong melt over a period of several days (Type B). In 11.7 ± 4.0%, Type A and B take place consecutively (Type C), and for 47.8 ± 6.8% no surface melt is observed at all (Type D). Continuous snowmelt is primarily observed in the outflow of the Weddell Gyre and in the northern Ross Sea, usually 17 days after the onset of temporary melt. Comparisons with Snow Buoy data suggest that also the onset of continuous snowmelt does not translate into changes in snow depth for a longer period but might rather affect the internal stratigraphy and density structure of the snowpack. Considering the entire data set, the timing of snowmelt processes does not show significant temporal trends.</jats:p>
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author Arndt, Stefanie, Willmes, Sascha, Dierking, Wolfgang, Nicolaus, Marcel
author_facet Arndt, Stefanie, Willmes, Sascha, Dierking, Wolfgang, Nicolaus, Marcel, Arndt, Stefanie, Willmes, Sascha, Dierking, Wolfgang, Nicolaus, Marcel
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container_issue 8
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description <jats:title>Abstract</jats:title><jats:p>An improved understanding of the temporal variability and the spatial distribution of snowmelt on Antarctic sea ice is crucial to better quantify atmosphere‐ice‐ocean interactions, in particular sea‐ice mass and energy budgets. It is therefore important to understand the mechanisms that drive snowmelt, both at different times of the year and in different regions around Antarctica. In this study, we combine diurnal brightness temperature differences (dT<jats:sub>B</jats:sub>(37 GHz)) and ratios (T<jats:sub>B</jats:sub>(19 GHz)/T<jats:sub>B</jats:sub>(37 GHz)) to detect and classify snowmelt processes. We distinguish temporary snowmelt from continuous snowmelt to characterize dominant melt patterns for different Antarctic sea‐ice regions from 1988/1989 to 2014/2015. Our results indicate four characteristic melt types. On average, 38.9 ± 6.0% of all detected melt events are diurnal freeze‐thaw cycles in the surface snow layer, characteristic of temporary melt (Type A). Less than 2% reveal immediate continuous snowmelt throughout the snowpack, i.e., strong melt over a period of several days (Type B). In 11.7 ± 4.0%, Type A and B take place consecutively (Type C), and for 47.8 ± 6.8% no surface melt is observed at all (Type D). Continuous snowmelt is primarily observed in the outflow of the Weddell Gyre and in the northern Ross Sea, usually 17 days after the onset of temporary melt. Comparisons with Snow Buoy data suggest that also the onset of continuous snowmelt does not translate into changes in snow depth for a longer period but might rather affect the internal stratigraphy and density structure of the snowpack. Considering the entire data set, the timing of snowmelt processes does not show significant temporal trends.</jats:p>
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spelling Arndt, Stefanie Willmes, Sascha Dierking, Wolfgang Nicolaus, Marcel 2169-9275 2169-9291 American Geophysical Union (AGU) Earth and Planetary Sciences (miscellaneous) Space and Planetary Science Geochemistry and Petrology Geophysics Oceanography http://dx.doi.org/10.1002/2015jc011504 <jats:title>Abstract</jats:title><jats:p>An improved understanding of the temporal variability and the spatial distribution of snowmelt on Antarctic sea ice is crucial to better quantify atmosphere‐ice‐ocean interactions, in particular sea‐ice mass and energy budgets. It is therefore important to understand the mechanisms that drive snowmelt, both at different times of the year and in different regions around Antarctica. In this study, we combine diurnal brightness temperature differences (dT<jats:sub>B</jats:sub>(37 GHz)) and ratios (T<jats:sub>B</jats:sub>(19 GHz)/T<jats:sub>B</jats:sub>(37 GHz)) to detect and classify snowmelt processes. We distinguish temporary snowmelt from continuous snowmelt to characterize dominant melt patterns for different Antarctic sea‐ice regions from 1988/1989 to 2014/2015. Our results indicate four characteristic melt types. On average, 38.9 ± 6.0% of all detected melt events are diurnal freeze‐thaw cycles in the surface snow layer, characteristic of temporary melt (Type A). Less than 2% reveal immediate continuous snowmelt throughout the snowpack, i.e., strong melt over a period of several days (Type B). In 11.7 ± 4.0%, Type A and B take place consecutively (Type C), and for 47.8 ± 6.8% no surface melt is observed at all (Type D). Continuous snowmelt is primarily observed in the outflow of the Weddell Gyre and in the northern Ross Sea, usually 17 days after the onset of temporary melt. Comparisons with Snow Buoy data suggest that also the onset of continuous snowmelt does not translate into changes in snow depth for a longer period but might rather affect the internal stratigraphy and density structure of the snowpack. Considering the entire data set, the timing of snowmelt processes does not show significant temporal trends.</jats:p> Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations Journal of Geophysical Research: Oceans
spellingShingle Arndt, Stefanie, Willmes, Sascha, Dierking, Wolfgang, Nicolaus, Marcel, Journal of Geophysical Research: Oceans, Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations, Earth and Planetary Sciences (miscellaneous), Space and Planetary Science, Geochemistry and Petrology, Geophysics, Oceanography
title Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_full Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_fullStr Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_full_unstemmed Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_short Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
title_sort timing and regional patterns of snowmelt on antarctic sea ice from passive microwave satellite observations
title_unstemmed Timing and regional patterns of snowmelt on Antarctic sea ice from passive microwave satellite observations
topic Earth and Planetary Sciences (miscellaneous), Space and Planetary Science, Geochemistry and Petrology, Geophysics, Oceanography
url http://dx.doi.org/10.1002/2015jc011504