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3 results for “COSMO-SkyMed”

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zenodo44/100

Rutford Ice Stream, Antarctica M_sf tidal velocity components derived from COSMO-SkyMED SAR data

<p>This repository provides rasters for&nbsp;velocity components of a&nbsp;tidal (periodic) model for Rutford Ice Stream (RIS), Antarctica. The tidal model consists of a secular (constant) term and a single sinusoidal component corresponding to the M_sf tidal cycle (14.76529 days). The tidal model is fit to time-dependent velocity fields over RIS derived from speckle tracking of COSMO-SkyMed&nbsp;SAR data, collected over 9 months beginning in August 2013.&nbsp;The original methodology and source dataset are described in the publication:</p> <p>Minchew, B. M., Simons, M., Riel, B., &amp; Milillo, P. (2017). Tidally induced variations in vertical and horizontal motion on Rutford Ice Stream, West Antarctica, inferred from remotely sensed observations.&nbsp;<em>Journal of Geophysical Research: Earth Surface</em>,&nbsp;<em>122</em>(1), 167-190. doi:&nbsp;<a href="https://doi.org/10.1002/2016JF003971">10.1002/2016JF003971</a></p> <p>The rasters are provided in GeoTIFF format in the Polar Stereographic South (EPSG: 3031) coordinate system. The velocity components are also referenced to Polar Stereographic South coordinates.&nbsp;The pixel spacing is 400 meters (in both the X- and Y-directions). The individual files are:</p> <ol> <li>vx_secular.tif: secular velocity in X-direction in meters/day.</li> <li>vy_secular.tif: secular velocity in Y-direction in meters/day.</li> <li>vx_amp.tif: M_sf velocity amplitude in X-direction in meters/day.</li> <li>vy_amp.tif: M_sf velocity amplitude in Y-direction in meters/day.</li> <li>vx_phase.tif: M_sf velocity phase delay in X-direction in days.</li> <li>vy_phase.tif: M_sf velocity phase delay in Y-direction in days.</li> </ol>

opencc-by-4.0Sep 2021View details →
zenodo40/100

Pre-eruption InSAR time-series at Kīlauea (Hawai`i, USA): COSMO-SkyMed Descending 2018

<p>InSAR time-series data for Kīlauea&nbsp;(Hawai`i, USA), between&nbsp;Jan 2010 and Sep 2011&nbsp;. Data were obtained by processing COSMO-SkyMed&nbsp;descending SAR data (track&nbsp;165). Data were processed using the JPL-developed InSAR Scientific Computing Environment (<code>ISCE</code>) open-source software package, and further time-series analysis was performed using the&nbsp;<code>MintPy</code>&nbsp;software toolbox (<a href="https://github.com/insarlab/MintPy">Miami INsar Time-series software in PYthon</a>), developed at the University of Miami.&nbsp;</p> <p>The following file&nbsp;is&nbsp;available in Hierarchical Data Format:</p> <p><code>geo_timeseries_tropHgt_demErr_cskDT165.h5</code>: Descending Track timeseries file.&nbsp;Dates available:</p> <p><code>[&#39;timeseries-20101001&#39;, &#39;timeseries-20101009&#39;, &#39;timeseries-20101017&#39;, &#39;timeseries-20101025&#39;, &#39;timeseries-20101102&#39;, &#39;timeseries-20101110&#39;, &#39;timeseries-20101118&#39;, &#39;timeseries-20101126&#39;, &#39;timeseries-20101204&#39;, &#39;timeseries-20101212&#39;, &#39;timeseries-20101220&#39;, &#39;timeseries-20110129&#39;, &#39;timeseries-20110206&#39;, &#39;timeseries-20110214&#39;, &#39;timeseries-20110222&#39;, &#39;timeseries-20110302&#39;, &#39;timeseries-20110303&#39;, &#39;timeseries-20110310&#39;, &#39;timeseries-20110318&#39;, &#39;timeseries-20110319&#39;, &#39;timeseries-20110322&#39;, &#39;timeseries-20110326&#39;, &#39;timeseries-20110403&#39;, &#39;timeseries-20110404&#39;, &#39;timeseries-20110407&#39;, &#39;timeseries-20110411&#39;, &#39;timeseries-20110419&#39;, &#39;timeseries-20110420&#39;, &#39;timeseries-20110423&#39;, &#39;timeseries-20110505&#39;, &#39;timeseries-20110506&#39;, &#39;timeseries-20110509&#39;, &#39;timeseries-20110513&#39;, &#39;timeseries-20110521&#39;, &#39;timeseries-20110522&#39;, &#39;timeseries-20110525&#39;, &#39;timeseries-20110529&#39;, &#39;timeseries-20110606&#39;, &#39;timeseries-20110607&#39;, &#39;timeseries-20110614&#39;, &#39;timeseries-20110622&#39;, &#39;timeseries-20110630&#39;, &#39;timeseries-20110708&#39;, &#39;timeseries-20110709&#39;, &#39;timeseries-20110716&#39;, &#39;timeseries-20110724&#39;, &#39;timeseries-20110725&#39;, &#39;timeseries-20110801&#39;, &#39;timeseries-20110809&#39;, &#39;timeseries-20110810&#39;, &#39;timeseries-20110817&#39;, &#39;timeseries-20110825&#39;, &#39;timeseries-20110826&#39;, &#39;timeseries-20110902&#39;, &#39;timeseries-20110910&#39;, &#39;timeseries-20110918&#39;]</code></p> <p>&nbsp;</p> <p>These data are supplemental to: Farquharson, J. I. and Amelung, F. [2020], &quot;<em>Extreme rainfall triggered the 2018 rift eruption at Kīlauea Volcano.</em>&quot;&nbsp;<a href="https://doi.org/10.1038/s41586-020-2172-5">https://doi.org/10.1038/s41586-020-2172-5</a></p>

opencc-by-4.0Jul 2020View details →
zenodo32/100

Automated grounding line delineation using deep learning and phase gradient-based approaches on COSMO-SkyMed DInSAR data

<p>This repository contains the file 'Natalya_Maslennikova_data_2024.zip,' which includes 171 DInSAR interferograms (both phase and coherence of a DInSAR signal) and three versions of the grounding lines: manually mapped ('gl_manual_mapping.shp'), mapped by the neural network ('gl_neural_network.shp'), and mapped using the phase gradient-based approach ('gl_phase_gradient.shp'). The X-band DInSAR data were acquired by the ASI&rsquo;s COSMO-SkyMed mission between 2020 and 2022 over five East Antarctica glaciers: Stancomb-Wills (STA: 32 interferograms), Veststraumen (VES: 35 interferograms), Jutulstraumen (JUT: 42 interferograms), Moscow University (MOS: 27 interferograms), and Rennick (REN: 35 interferograms).</p> <p>The 'gl_neural_network.shp' and 'gl_phase_gradient.shp' shapefiles contain the following fields: the name of the glacier (the 'Glacier' column), four dates in YYYYMMDD format when the corresponding DInSAR interferogram was acquired (the 'Primary1', 'Secondary1', 'Primary2', 'Secondary2' columns), and the double difference name in 'Primary1_Secondary1-Primary2_Secondary2' format (the 'DD' column). The 'gl_manual_mapping.shp' shapefile contains 'Glacier', 'Primary1', 'Secondary1', 'Primary2', 'Secondary2', and 'DD' columns as well, along with the 'Revisit' column (difference in days between the 'Primary1' and 'Primary2' images were acquired), the 'Time' column (acquisition time in 'HHMMSS' format), the 'Coherence' column (average coherence of the corresponding DInSAR interferogram), and the 'Train_1', 'Train_2', 'Train_3' columns, which contain indicators 'Y' for 'yes' and 'N' for 'no', showing whether or not the DInSAR interferogram was used in the corresponding training session.</p>

opencc-by-4.0May 2024View details →

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