IGARSS 2018 - 2018 IEEE International Geoscience and Remote Sensing Symposium 2018
DOI: 10.1109/igarss.2018.8517785
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Prisma Hyperspectral Mission Products

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Cited by 31 publications
(16 citation statements)
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“…Launched on 22 March 2019, the PRISMA pushbroom sensor has 239 hyperspectral bands in a spectral range between 400-2500 nm with 30 m of spatial resolution (5 m for Panchromatic band), and a revisit time of approximately 29 days. Of the 239 bands, 66 correspond to Visible and Near Infrared region (VNIR: 400-1010 nm) and 173 to the Short Wave Infrared region (SWIR: 920-2505 nm) spectrum 1,11 . A product collected on 05/04/2020, with a cloud coverage of 3,27% was downloaded from the PRISMA Mission Catalog website (https://prisma.asi.it/).…”
Section: Data and Preprocessingmentioning
confidence: 99%
“…Launched on 22 March 2019, the PRISMA pushbroom sensor has 239 hyperspectral bands in a spectral range between 400-2500 nm with 30 m of spatial resolution (5 m for Panchromatic band), and a revisit time of approximately 29 days. Of the 239 bands, 66 correspond to Visible and Near Infrared region (VNIR: 400-1010 nm) and 173 to the Short Wave Infrared region (SWIR: 920-2505 nm) spectrum 1,11 . A product collected on 05/04/2020, with a cloud coverage of 3,27% was downloaded from the PRISMA Mission Catalog website (https://prisma.asi.it/).…”
Section: Data and Preprocessingmentioning
confidence: 99%
“…PRISMA is a medium-resolution hyperspectral imaging mission of the Italian Space Agency that was launched in March 2019 [74]. The PRISMA sensor is a spaceborne system that acquires hyperspectral datasets continuously, with a repeat orbital cycle of approximately 29 days [75].…”
Section: Prisma Imagesmentioning
confidence: 99%
“…The PRISMA data are made available for free by the Italian Space Agency (ASI) [23,28]. The data are delivered in the HDF5 format with four options: (1) Level 1 (Hyperspectral/PAN) is radiometrically corrected and calibrated TOA (top of atmosphere) data;…”
Section: Prisma Scenementioning
confidence: 99%
“…We used the LC1-PRISMA product acquired on 27 December 2019. The image processing was implemented by using the ENVI 5.5 (Harris Geospatial Solution, USA) software and consisted of three steps: (1) applying the scale factor 100 to convert the digital numbers of the L1 product to radiance expressed in Wm −2 sr −1 µm −1 [23,28]; (2) removing noisy bands and building the hyperspectral cube, by stacking the visible and SWIR data; (3) implementing the atmospheric correction and obtaining a reflectance spectrum; (4) producing spectral detection maps and implementing the code (in Matlab 2020b) for the semi-automatic processing of the CO 2 -CIBR and HDFI. The hypercube was visually explored to identify the noisy bands affecting the spectra; specifically, the bands within two VNIR spectral intervals (402.2041-426.7687 nm and 972.3630-959.4313 nm) and two SWIR intervals (942.8875-969.7985 nm and 2456.2781-2496.8254 nm) were removed.…”
Section: Prisma Scenementioning
confidence: 99%