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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Main Authors: Hollands, Thomas, Dierking, Wolfgang, Höppner, Kathrin, Wachter, Paul
Format: Conference Object
Language:unknown
Published: WSL Institute for Snow and Avalanche Research SLF 2018
Subjects:
Online Access: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
id ftawi:oai:epic.awi.de:47433
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spelling 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)
institution Open Polar
collection Alfred Wegener Institute for Polar- and Marine Research (AWI): ePIC (electronic Publication Information Center)
op_collection_id ftawi
language unknown
description 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
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