Flight Performance of the AKARI Cryogenic System
arXiv:0708.1797 · doi:10.1093/pasj/59.sp2.S377
Abstract
We describe the flight performance of the cryogenic system of the infrared astronomical satellite AKARI, which was successfully launched on 2006 February 21 (UT). AKARI carries a 68.5 cm telescope together with two focal plane instruments, Infrared Cameras (IRC) and Far Infrared Surveyor (FIS), all of which are cooled down to cryogenic temperature to achieve superior sensitivity. The AKARI cryogenic system is a unique hybrid system, which consists of cryogen (liquid helium) and mechanical coolers (2-stage Stirling coolers). With the help of the mechanical coolers, 179 L (26.0 kg) of super-fluid liquid helium can keep the instruments cryogenically cooled for more than 500 days. The on-orbit performance of the AKARI cryogenics is consistent with the design and pre-flight test, and the boil-off gas flow rate is as small as 0.32 mg/s. We observed the increase of the major axis of the AKARI orbit, which can be explained by the thrust due to thermal pressure of vented helium gas.
19 pages, 10 figures, and 6 tables. Accepted for publication in the AKARI special issue of the Publications of the Astronomical Society of Japan
References in corpus (5)
Cited by in corpus (16)
- The Infrared Astronomical Mission AKARI
- The Infrared Camera (IRC) for AKARI - Design and Imaging Performance
- The Far-Infrared Surveyor (FIS) for AKARI
- The Far-Infrared All-Sky Survey Maps
- Calibration and Performance of the AKARI Far-Infrared Surveyor (FIS) -- Slow-Scan Observation Mode for Point Sources
- Calibration of the AKARI Far-infrared All Sky Survey Maps
- The AKARI FIS YSO Catalogue
- In-orbit focal adjustment of the AKARI telescope with IRC images
- AKARI infrared imaging of reflection nebulae IC4954 and IC4955
- Performance of the Imaging Fourier Transform Spectrometer with Photoconductive Detector Arrays: An Application for the AKARI Far-Infrared Instrument
- Low-Resolution Spectrum of the Zodiacal Light with AKARI InfraRed Camera
- A Comparative Study of Infrared Asteroid Surveys: IRAS, AKARI, and WISE
- Revised Wavelength and Spectral Response Calibrations for AKARI Near-Infrared Grism Spectroscopy: Cryogenic Phase
- SPICA infrared coronagraph for the direct observation of exo-planets
- Radio-Infrared Correlation for Local Dusty Galaxies and Dusty AGNs from the AKARI All Sky Survey
- Dense Molecular Cores Being Externally Heated