AVIRIS-4 Hyperspectral
Measures solar reflected radiance from 380 to 2510 nm in 224 contiguous spectral bands. Used for mineral mapping, canopy chemistry, and snow hydrology.
🚀 Atmospheric Layer Physics
The ER-2 routinely traverses the tropopause (approx. 36,000–40,000 ft in mid-latitudes), penetrating deep into the stable, dry stratosphere. In this layer, ambient pressure falls below 60 hPa (0.87 psi), leaving over 94% of Earth's atmospheric mass below the aircraft, creating pristine conditions for astronomical and hyperspectral remote sensing.
⚠️ The "Coffin Corner" Regime
As altitude increases, true airspeed (TAS) must remain high to generate sufficient dynamic pressure (q = ½ρV²) on the ER-2's 103-foot wingspan. Simultaneously, the speed of sound drops due to colder temperatures. The narrow corridor where stall speed (Vs) approaches critical Mach buffet (Mmo) is known as the Coffin Corner—requiring extreme pilot precision and U-2/ER-2 full pressure suits.
🛰️ Satellite Calibration & In-Situ Chemistry
Operating as a surrogate satellite platform from Armstrong Flight Research Center (AFRC Building 703 in Palmdale, CA), ER-2 flights validate sensors for NASA Earth observing satellites (PACE, Landsat, Sentinel, TEMPO) and directly collect chlorofluorocarbon (CFC) breakdown products, stratospheric ozone, and volcanic sulfate aerosols.
Download complete mission telemetry profiles including 1976 US Standard Atmosphere metrics, aerodynamic limits, and sensor swath geometries for mission planning or GIS analysis.