HIgh Resolution Mid-infrarEd Spectrometer (HIRMES) is a facility-class instrument aboard the Stratospheric Observatory for Infrared Astronomy (SOFIA) Aircraft Observatory. A TransMIT PTD 406C pulse tube cryocooler (PTC) is used to cool the optical bench and optical components to 4K. A second PTC is dedicated to cool the 3He/4He sorption cooler. The first stages of the PTCs share the heat load from the intermediate temperature stage. The second stage of the first PTC removes nearly all the heat load from the 4 degrees Kelvin stage. The results of thermal analysis show that the 4 degrees Kelvin stage of the HIRMES thermal subsystem meets all of its requirements using the 100 percent heat load margin approach and conservative modeling assumpti...
The quest for knowledge and the initiative to solve the mysteries around us entail to develop instru...
The characteristics of a cryogenic cooling system for the Pollution Monitoring Satellite (PMS) are d...
A brief summary from the 1985 Large Deployable Reflector (LDR) Asilomar 2 workshop of the requiremen...
Astronomy at infrared wavelengths requires optical instruments that operate at low temperatures, whi...
The NASA Astrophysics Division has commissioned 4 studies for consideration by the 2020 Decadal Surv...
This paper presents a description of the Hubble Space Telescope (HST) Near-Infrared Camera and Multi...
A program to detect and monitor the presence of trace constituents in the earth's atmosphere by usin...
The Origins Space Telescope (OST) concept is one of four NASA Science Mission Directorate, Astrophys...
The MUSCAT instrument is a large-format camera planned for installation on the Large Millimeter Tele...
The Mid Infrared Instrument (MIRI) on the James Webb Space Telescope includes a mechanical cryocoole...
In 2017, the combined Optical Telescope Element and Integrated Science Instrument Module (OTIS) of t...
The focus of this research is on the reduction of the refrigeration requirements for infrared sensor...
Presented at the 16th International Cryocooler Conference, held May 17-20, 2008 in Atlanta, Georgia....
The Thermal Infrared Sensor (TIRS) is an instrument on Landsat 8, launched in February 2013. The foc...
Future astronomical instruments will require sub-Kelvin detector temperatures to obtain high sensiti...
The quest for knowledge and the initiative to solve the mysteries around us entail to develop instru...
The characteristics of a cryogenic cooling system for the Pollution Monitoring Satellite (PMS) are d...
A brief summary from the 1985 Large Deployable Reflector (LDR) Asilomar 2 workshop of the requiremen...
Astronomy at infrared wavelengths requires optical instruments that operate at low temperatures, whi...
The NASA Astrophysics Division has commissioned 4 studies for consideration by the 2020 Decadal Surv...
This paper presents a description of the Hubble Space Telescope (HST) Near-Infrared Camera and Multi...
A program to detect and monitor the presence of trace constituents in the earth's atmosphere by usin...
The Origins Space Telescope (OST) concept is one of four NASA Science Mission Directorate, Astrophys...
The MUSCAT instrument is a large-format camera planned for installation on the Large Millimeter Tele...
The Mid Infrared Instrument (MIRI) on the James Webb Space Telescope includes a mechanical cryocoole...
In 2017, the combined Optical Telescope Element and Integrated Science Instrument Module (OTIS) of t...
The focus of this research is on the reduction of the refrigeration requirements for infrared sensor...
Presented at the 16th International Cryocooler Conference, held May 17-20, 2008 in Atlanta, Georgia....
The Thermal Infrared Sensor (TIRS) is an instrument on Landsat 8, launched in February 2013. The foc...
Future astronomical instruments will require sub-Kelvin detector temperatures to obtain high sensiti...
The quest for knowledge and the initiative to solve the mysteries around us entail to develop instru...
The characteristics of a cryogenic cooling system for the Pollution Monitoring Satellite (PMS) are d...
A brief summary from the 1985 Large Deployable Reflector (LDR) Asilomar 2 workshop of the requiremen...