PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay
Satellite images provide the opportunity to differentiate different ice units in and around the Terra Nova Bay Polynya (TNBP) in the Ross Sea (Antarctica) on different spatial scales. However, at a first stage, the separation of units is usually be carried out in terms of radar signature variations,...
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ftawi:oai:epic.awi.de:47433 2024-09-15T17:41:57+00:00 PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay Hollands, Thomas Dierking, Wolfgang Höppner, Kathrin Wachter, Paul 2018-06-20 application/pdf https://epic.awi.de/id/eprint/47433/ https://epic.awi.de/id/eprint/47433/1/Hollands1774.pdf https://www.polar2018.org/uploads/2/4/6/0/24605948/polar2018_abstractproceedings.pdf https://hdl.handle.net/10013/epic.ffa49176-d866-4c91-bfd9-10631ddeb932 unknown WSL Institute for Snow and Avalanche Research SLF https://epic.awi.de/id/eprint/47433/1/Hollands1774.pdf Hollands, T. orcid:0000-0003-0824-4037 , Dierking, W. orcid:0000-0002-5031-648X , Höppner, K. and Wachter, P. (2018) PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay , Open Science Conference, Davos, Switzerland, 19 June 2018 - 23 June 2018 . hdl:10013/epic.ffa49176-d866-4c91-bfd9-10631ddeb932 EPIC3Open Science Conference, Davos, Switzerland, 2018-06-19-2018-06-23Davos, Switzerland, WSL Institute for Snow and Avalanche Research SLF Conference notRev 2018 ftawi 2024-06-24T04:19:47Z Satellite images provide the opportunity to differentiate different ice units in and around the Terra Nova Bay Polynya (TNBP) in the Ross Sea (Antarctica) on different spatial scales. However, at a first stage, the separation of units is usually be carried out in terms of radar signature variations, i. e. the result are “radar units” with statistically significant signature differences. In a second step, the radar units have to be linked to observations in the field in order to enable a geophysical interpretation of the stage of polynya development and the sea ice conditions around the polynya. In this specific analysis we focus on the first step. The radar imagery acquired over the TNBP comprises data from TerraSAR-X strip-map dual-polarization (HH, VV) mode, TerraSAR-X ScanSAR mode (HH-polarization), Sentinel-1 extra wide-swath mode (HH and HV polarization), and Sentinel-1 interferometric wide-swath mode (HH-polarization). Dependent on the temporal gap between image acquisitions it is possible in some cases to produce layer stacks including different imaging modes. We use different segmentation methods (such as e. g. Support Vector Machine) to arrive at a map of different radar units with only small overlaps of their radar signatures (i. e. significant discernibility). The goal is to generate a temporal sequence of radar unit maps, which in the second step in collaboration with the PIPERS team can be related to ground data gathered in the field. Conference Object Antarc* Antarctica Ross Sea Sea ice Alfred Wegener Institute for Polar- and Marine Research (AWI): ePIC (electronic Publication Information Center) |
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Open Polar |
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Alfred Wegener Institute for Polar- and Marine Research (AWI): ePIC (electronic Publication Information Center) |
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ftawi |
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Satellite images provide the opportunity to differentiate different ice units in and around the Terra Nova Bay Polynya (TNBP) in the Ross Sea (Antarctica) on different spatial scales. However, at a first stage, the separation of units is usually be carried out in terms of radar signature variations, i. e. the result are “radar units” with statistically significant signature differences. In a second step, the radar units have to be linked to observations in the field in order to enable a geophysical interpretation of the stage of polynya development and the sea ice conditions around the polynya. In this specific analysis we focus on the first step. The radar imagery acquired over the TNBP comprises data from TerraSAR-X strip-map dual-polarization (HH, VV) mode, TerraSAR-X ScanSAR mode (HH-polarization), Sentinel-1 extra wide-swath mode (HH and HV polarization), and Sentinel-1 interferometric wide-swath mode (HH-polarization). Dependent on the temporal gap between image acquisitions it is possible in some cases to produce layer stacks including different imaging modes. We use different segmentation methods (such as e. g. Support Vector Machine) to arrive at a map of different radar units with only small overlaps of their radar signatures (i. e. significant discernibility). The goal is to generate a temporal sequence of radar unit maps, which in the second step in collaboration with the PIPERS team can be related to ground data gathered in the field. |
format |
Conference Object |
author |
Hollands, Thomas Dierking, Wolfgang Höppner, Kathrin Wachter, Paul |
spellingShingle |
Hollands, Thomas Dierking, Wolfgang Höppner, Kathrin Wachter, Paul PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay |
author_facet |
Hollands, Thomas Dierking, Wolfgang Höppner, Kathrin Wachter, Paul |
author_sort |
Hollands, Thomas |
title |
PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay |
title_short |
PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay |
title_full |
PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay |
title_fullStr |
PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay |
title_full_unstemmed |
PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay |
title_sort |
pipers: preliminary analysis of satellite radar imagery from terra nova bay |
publisher |
WSL Institute for Snow and Avalanche Research SLF |
publishDate |
2018 |
url |
https://epic.awi.de/id/eprint/47433/ https://epic.awi.de/id/eprint/47433/1/Hollands1774.pdf https://www.polar2018.org/uploads/2/4/6/0/24605948/polar2018_abstractproceedings.pdf https://hdl.handle.net/10013/epic.ffa49176-d866-4c91-bfd9-10631ddeb932 |
genre |
Antarc* Antarctica Ross Sea Sea ice |
genre_facet |
Antarc* Antarctica Ross Sea Sea ice |
op_source |
EPIC3Open Science Conference, Davos, Switzerland, 2018-06-19-2018-06-23Davos, Switzerland, WSL Institute for Snow and Avalanche Research SLF |
op_relation |
https://epic.awi.de/id/eprint/47433/1/Hollands1774.pdf Hollands, T. orcid:0000-0003-0824-4037 , Dierking, W. orcid:0000-0002-5031-648X , Höppner, K. and Wachter, P. (2018) PIPERS: Preliminary Analysis of Satellite Radar Imagery from Terra Nova Bay , Open Science Conference, Davos, Switzerland, 19 June 2018 - 23 June 2018 . hdl:10013/epic.ffa49176-d866-4c91-bfd9-10631ddeb932 |
_version_ |
1810488274558386176 |