Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Hans, Courrier"'
Autor:
Warren Davis, Constantine Lukashin, Michael Stebbins, Christine Buleri, Michael Cooney, Greg Kopp, Trevor Jackson, Michael Kehoe, Paul Smith, Thomas C. Stone, Hans Courrier, Rand Swanson
Publikováno v:
2020 IEEE Aerospace Conference.
The purpose of the ARCSTONE project is to more accurately measure the spectral lunar reflectance so the Moon can be used as a high-accuracy SI-traceable exo-atmospheric calibration standard for Earth-viewing instruments in low-Earth orbits. The spect
Publikováno v:
Imaging and Applied Optics Congress.
Most push-broom hyperspectral imagers rely on circularly symmetric optics that require tradeoffs between spatial and spectral performance. Introducing anamorphic optics provides additional engineering freedom to mitigate the tradeoffs for improved op
Publikováno v:
Solar Physics. 293
Using the 2016 Mercury transit of the Sun, we characterize on orbit spatial point spread functions (PSFs) for the Near- (NUV) and Far- (FUV) Ultra-Violet spectrograph channels of NASA’s Interface Region Imaging Spectrograph (IRIS). A semi-blind Ric
Publikováno v:
Solar Physics
Using the 2016 Mercury transit of the Sun, we characterize on orbit spatial point spread functions (PSFs) for the Near- (NUV) and Far- (FUV) Ultra-Violet spectrograph channels of NASA’s Interface Region Imaging Spectrograph (IRIS). A semi-blind Ric
Autor:
Charles C. Kankelborg, Hans Courrier
Publikováno v:
Journal of Astronomical Telescopes, Instruments, and Systems. 4:1
The Multi-Order Solar EUV Spectrograph (MOSES) is a sounding rocket instrument that utilizes a concave spherical diffraction grating to form simultaneous images in the diffraction orders m=0, +1, and −1. MOSES is designed to capture high-resolution
Autor:
Charles C. Kankelborg, Hans Courrier
Publikováno v:
SPIE Proceedings.
The Multi-Order Solar EUV Spectrograph (MOSES) is a sounding rocket instrument that utilizes a concave spherical diffraction grating to form simultaneous solar images in the diffraction orders m = 0, +1, and −1. The large 2D field of view allows a