spectral analysis
The WSO (Wilcox Solar Observatory at Stanford University) terrestrial observatory data, spanning 47 years of solar Mean Magnetic Field (MMF) values. The set also includes data from the WIND space mission's magnetometer (MAG), collected at the L1 Lagrangian point over the time interval of 27 years.
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This dataset (samplePointsCities_20240811_harmonized.csv) was used for the Rescaled Water Index (RWI) proposal. The GitHub page (https://github.com/edujusti/Rescaled-Water-Index-RWI) contains the Python and JavaScript (Google Earth Engine) scripts used for data production, statistical analyses, and result visualization of the RWI spectral index.
This spectral index is a modification of MNDWI to enhance the mappings of water surfaces.
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The "CloudPatch-7 Hyperspectral Dataset" comprises a manually curated collection of hyperspectral images, focused on pixel classification of atmospheric cloud classes. This labeled dataset features 380 patches, each a 50x50 pixel grid, derived from 28 larger, unlabeled parent images approximately 4402-by-1600 pixels in size. Captured using the Resonon PIKA XC2 camera, these images span 462 spectral bands from 400 to 1000 nm.
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El carbono orgánico (OC) y el nitrógeno total (N) son
Nutrientes sensibles para el crecimiento de las plantas. La presencia de estos nutrientesEl carbono orgánico (OC) y el nitrógeno total (N) sonOrganic carbon (OC) and total nitrogen (N) are es-Organic carbon (OC) and total nitrogen (N) are sential nutrients for plant growth. The presence of these nutrierganic carbon (OC) and total nitrogen (N) are ews-
w
sential nutrients for plant growth. The presence of these nutrients
in acceptable quantities can generate an optimal environment for
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Mission-integrated ⪅8nT magnetometer (MAG) data at Jupiter and Saturn, 100-minute averages. Data consist of the only available MAG measurements that spanned at least 6 months (180 Earth days), and include the Cassini–Huygens, Galileo, and Juno missions. Steven P. Joy and Joe Mafi (UCLA & NASA Planetary Data System/Planetary Plasma Interactions Node) provided concatenated and RTN-rotated Jupiter MAG 1-minute averages from Galileo and Juno, including random samples of field swelling.
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North/South-separated <10nT magnetometer data from the 1994-2008 Ulysses space mission's samplings of polar solar winds, hourly averaged, non-decimated. The set also includes data from the WIND space mission, the WSO terrestrial observatory (solar Mean Magnetic Field), and the WSO solar Polar magnetic Field, all used in the same research project. The NOAA Solar Indices data (not included) were used for verification, see paper for details.
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