๐ช๐ต๐ถ๐ฐ๐ต ๐๐ฎ๐๐ฒ๐น๐น๐ถ๐๐ฒ ๐ฝ๐ฟ๐ผ๐๐ถ๐ฑ๐ฒ๐ฟ๐ ๐ฎ๐ป๐ฑ ๐ถ๐บ๐ฎ๐ด๐ฒ๐ฟ๐ ๐ฝ๐ฟ๐ผ๐ฑ๐๐ฐ๐๐ ๐ฎ๐ฟ๐ฒ ๐๐๐ฝ๐ฝ๐ผ๐ฟ๐๐ฒ๐ฑ ๐ฏ๐ ๐ฆ๐ธ๐๐๐ถ?


SkyFi aggregates imagery from multiple satellite providers and offers various product types (sensor modalities). When searching or ordering, you will encounter the following options:
๐ฃ๐ฟ๐ผ๐๐ถ๐ฑ๐ฒ๐ฟ๐ / ๐๐ผ๐ป๐๐๐ฒ๐น๐น๐ฎ๐๐ถ๐ผ๐ป๐:
The provider field or filter can include (but is not limited to) the following:
๐๐๐๐๐ (๐๐๐๐๐๐๐๐๐)โ High-resolution optical satellites.
๐๐ผ๐๐๐๐๐๐๐๐พ โ High-frequency imaging constellation (optical).
๐๐๐ฝ๐๐ผ โ Synthetic Aperture Radar (SAR) provider.
๐๐ผ๐๐๐๐๐๐ฟ, ๐๐๐๐๐ผ๐ โ Other optical imagery providers.
๐๐๐๐๐๐๐๐2 (๐ซ๐๐ ๐พ๐๐๐๐ฟ๐๐ผ๐)โ Sentinel-2 open data imagery (multispectral, 10m resolution, free).
๐๐๐ผ๐๐๐ โ Planet Labs imagery (high revisit optical).
๐๐๐๐๐, ๐๐๐ฝ๐ผ๐_๐๐๐, ๐๐๐, ๐๐๐๐พ๐๐ โ Additional providers (covering various types from stratospheric imagery to aerial or others, as integrated by SkyFi).
๐ฃ๐ฟ๐ผ๐ฑ๐๐ฐ๐ ๐ง๐๐ฝ๐ฒ๐: This refers to the type of data or sensor:
๐ฟ๐ผ๐ โ Daytime optical imagery (true color/RGB and possibly near-infrared; standard satellite photos in daylight).
๐๐๐๐๐ โ Nighttime optical imagery (low-light imaging at night).
๐๐๐ฟ๐๐ โ Satellite video footage (some providers can capture short video clips of an area).
๐๐๐๐๐๐๐๐๐พ๐๐๐ผ๐ โ Multi-band imagery (e.g., Sentinel-2 or high-res satellites with multiple spectral bands).
๐๐๐๐๐๐๐๐๐พ๐๐๐ผ๐ โ Hyperspectral imagery (many narrow spectral bands, typically special sensors).
๐๐ผ๐ โ Synthetic Aperture Radar imagery (radar-based imaging, can see through clouds, day/night).
๐๐๐๐๐๐ โ Stereoscopic image pairs for 3D elevation extraction.
๐ฅ๐ฒ๐๐ผ๐น๐๐๐ถ๐ผ๐ป ๐๐ฎ๐๐ฒ๐ด๐ผ๐ฟ๐ถ๐ฒ๐: The API categorizes resolution into bands:
LOW, MEDIUM, HIGH, VERY HIGH, SUPER HIGH, ULTRA HIGH, and specific centimeter classes (e.g., CM 30, CM 50).
These categories correspond to the ground sampling distance (GSD):
Low might be 10 m per pixel (e.g., Sentinel-2).
High could be around 1 m per pixel.
Very High/Super/Ultra High implies sub-meter resolutions (e.g., 30 cm or 50 cm per pixel or better).
Each archive record will indicate its resolution category and often provide the exact GSD in centimeters (platformResolution or gsd field).
In summary, the SkyFi API acts as a one-stop interface to access many satellite constellations. You can specify exactly what kind of imagery you need (e.g., โI need a high-resolution SAR image from Umbraโ or โa low-resolution multispectral image from Sentinel-2โ) and the API will handle the request to the appropriate provider.
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