Time assignment system and its performance aboard the Hitomi satellite

Abstract. Fast timing capability in x-ray observation of astrophysical objects is one of the key properties for the ASTRO-H (Hitomi) mission. Absolute timing accuracies of 350 or 35  μs are required to achieve nominal scientific goals or to study fast variabilities of specific sources. The satellite carries a GPS receiver to obtain accurate time information, which is distributed from the central onboard computer through the large and complex SpaceWire network. The details of the time system on the hardware and software design are described. In the distribution of the time information, the propagation delays and jitters affect the timing accuracy. Six other items identified within the timing system will also contribute to absolute time error. These error items have been measured and checked on ground to ensure the time error budgets meet the mission requirements. The overall timing performance in combination with hardware performance, software algorithm, and the orbital determination accuracies, etc. under nominal conditions satisfies the mission requirements of 35  μs. This work demonstrates key points for space-use instruments in hardware and software designs and calibration measurements for fine timing accuracy on the order of microseconds for midsized satellites using the SpaceWire (IEEE1355) network.

[1]  Yoshitaka Ishisaki,et al.  In-Orbit Timing Calibration of the Hard X-Ray Detector on Board Suzaku , 2008 .

[2]  Tadayuki Takahashi,et al.  Soft gamma-ray detector (SGD) onboard the ASTRO-H mission , 2014, Astronomical Telescopes and Instrumentation.

[3]  Steve Parkes,et al.  SpaceWire-D: Deterministic Data Delivery Over SpaceWire , 2014 .

[4]  Hiroshi Nakajima,et al.  Soft X-ray Imager (SXI) onboard ASTRO-H , 2014, Astronomical Telescopes and Instrumentation.

[5]  Matteo Guainazzi,et al.  Hitomi X-ray studies of Giant Radio Pulses from the Crab pulsar. , 2017, Publications of the Astronomical Society of Japan. Nihon Tenmon Gakkai.

[6]  Tadayuki Takahashi,et al.  The time assignment system of ASTRO-H , 2011, 2011 IEEE Nuclear Science Symposium Conference Record.

[7]  Motohide Kokubun,et al.  SPACEWIRE DRIVEN ARCHITECTURE FOR THE ASTRO-H SATELLITE Session : SpaceWire Missions and Applications Long Paper , 2010 .

[8]  Yoshiharu Namba,et al.  The ASTRO-H (Hitomi) x-ray astronomy satellite , 2016, Astronomical Telescopes + Instrumentation.

[9]  Stephen S. Murray,et al.  Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray , 2010 .

[10]  Ryuichi Fujimoto,et al.  The high-resolution x-ray microcalorimeter spectrometer system for the SXS on ASTRO-H , 2010, Astronomical Telescopes + Instrumentation.

[11]  Steve Parkes The Operation and Uses of the SpaceWire Time-Code International SpaceWire Seminar (ISWS 2003) , 2003 .

[12]  Steve Parkes SpaceWire Remote Memory Access Protocol , 2005 .

[13]  Tadayuki Takahashi,et al.  The Hard X-ray Imager (HXI) for the ASTRO-H mission , 2012, Other Conferences.

[14]  Yasuo Tanaka,et al.  The X-Ray Astronomy Satellite ASCA (Initial Results from ASCA) , 1994 .

[15]  B. Schlesinger,et al.  Definition of the Flexible Image Transport System (FITS) , 2001 .