Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Jed Diller"'
Autor:
Jed Diller, Randy Rose, Jillian Redfern, Michael Vincent, Debi Rose, Zach Dischner, Kerry Wahl, Christopher S. Ruf
Publikováno v:
SpaceOps 2016 Conference.
Autor:
Michael W. Davis, Craig DeForest, Thomas R. Ayres, Roy Graham, Jed Diller, David D. Slater, Roger J. Thomas, Donald M. Hassler, Harry P. Warren, Bart De Pontieu, Glenn Laurent, Udo Schuele, Harald Michaelis
Publikováno v:
Journal of Astronomical Instrumentation.
We present a summary of the solar observing Rapid Acquisition Imaging Spectrograph Experiment (RAISE) sounding rocket program including an overview of the design and calibration of the instrument, flight performance, and preliminary chromospheric res
Publikováno v:
2015 IEEE Aerospace Conference.
The SwRI Solar Instrument Pointing Platform (SSIPP) is a protoflight system that leverages the low cost, reusability of suborbital vehicles. SSIPP enables observatory-like solar instrument development at a fraction of the cost and risk of traditional
Publikováno v:
2015 IEEE Aerospace Conference.
In September, 2013 the BRRISON mission suffered an anomaly resulting in a total loss of science data for the duration of flight. The Balloon Observation Platform for Planetary Science (BOPPS) mission is in essence a re-flight of the BRRISON mission.
Publikováno v:
2014 IEEE Aerospace Conference.
Balloon-borne telescopes have the potential to provide space-quality imaging. However, long exposures require pointing stability on the order of the optical point spread function (PSF). Consequently, one of the main goals of the BRRISON (Balloon Rapi
Publikováno v:
2014 IEEE Aerospace Conference.
Open source tools and readily available consumer hardware offer many advantages over the typical, custom designs used for control and data handling (CDH) and electronic power systems (EPS), especially in applications where the development time is mea
Publikováno v:
2013 IEEE Aerospace Conference.
High altitude balloons are capable of supporting astronomical observations with virtually no image degradation due to atmospheric turbulence. To take advantage of this space-like seeing, a telescope must be pointed and stabilized with sub-arcsecond p