Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.cplire.ru/html/lab234/pubs/2011_07a.pdf Дата изменения: Fri Sep 9 23:23:12 2011 Дата индексирования: Tue Oct 2 09:24:04 2012 Кодировка: Поисковые слова: milky way

Operating of the superconducting integrated receiver channel of the TELIS atmospheric sounder.
O. S. Kiselev1, M. Birk2, P. N. Dmitriev1, A. B. Ermakov1, L. V. Filippenko1, H. Golstein3, B. van Kuik3, A. de Lange3, G. De Lange3, A. M. Selig3, P. Vogt2, G. Wagner2, and V. P. Koshelets1
1

Kotel'nikov Institute of Radio Engineering and Electronics IREE, Moscow, Russia 2 DLR German Aerospace Centre, Wessling, Germany 3 SRON Netherlands Institute for Space Research, Groningen, the Netherlands

Abstract
A Superconducting Integrated Receiver (SIR) was proposed more than 15 years ago and has since then been developed up to the point of practical applications. We have demonstrated for the first time the capabilities of the SIR technology for heterodyne spectroscopy both in the laboratory and at remote operation under harsh environmental conditions for atmospheric research. Within a SIR the main components needed for a superconducting heterodyne receiver such as an SIS-mixer with quasioptical antenna, a Flux-Flow oscillator (FFO) as the local oscillator, and a harmonic mixer to phase-lock the FFO are integrated on a single chip. Light weight and low power consumption combined with broadband operation and nearly quantum limited sensitivity make the SIR a perfect candidate for future airborne and space-borne missions. The noise temperature of the SIR was measured to be as low as 120 K, with an intermediate frequency band of 4 ­ 8 GHz in double sideband operation; the spectral resolution is well below 1 MHz. The SIR was implemented in the three-channel balloon-borne instrument TELIS (TErahertz and submillimeter LImb Sounder) that detects spectral emission lines of stratospheric trace gases (like ClO and BrO). These gases even in small quantities can have a significant impact on the atmosphere because they speed up certain chemical processes, such as ozone depletion. The SIR is very sensitive to external electromagnetic interference and temperature variations, but specially developed shielding, novel design of the SIR itself and sophisticated operating algorithms provide stable operation of the device. During the flight the SIR should perform extremely stable and reliable ­ some measurements last about an hour. The changing of the LO frequency for next measurement should be as fast as possible (about 1 min).

TELIS
TErahertz and submm LImb Sounder
· · Balloon instrument on board MIPAS B2 gondola, IMK Karlsruhe Three independent frequency channels, cryogenic heterodyne receivers: ­ ­ ­ 500 GHz by RAL (UK) 450-650 GHz by SRON-IREE 1.8 THz by DLR (PI-institute)

Remote SIR operation
The SIR channel is controlled with a batteryoperated ultra low noise biasing system. The SIR bias unit is digitally controlled by the onboard DLR PC-104 computer, that also interfaces with the other channels, the digital autocorrelator, and with the host instrument MIPAS. A radio link provides real-time two-way contact with the ground segment consisting of a server computer with three dedicated client computers, coupled through TCP/IP socket connections. The complete system is designed to have sufficient battery power for a 24 hour flight. Special procedures for pre-flight tests and remote operation during the flight had been developed and tested

TELIS Objectives:
· Measure many species for atmospheric science: ClO, BrO, O3, HCl, HOCl, etc; · Chemistry, Transport, Climate · Serve as a test platform for new sensors · Serve as validation tool for future satellite missions

Communication scheme of the TELIS-SIR flight electronics

Operator
Database

CNES

Ground segment ment of the control system

Server Radio channel

Gondola

CNES

PC 104 Linux

TSCU Autocorrelator

TELIS instrument model

TELIS-SIR Main Parameters
Block Diagram of the Superconducting Integrated Receiver

#
1 2 3 4 5 6

LH e C r yost at S I R M i c r o c ir c u it s
SI S - m i x e r w i t h plan ar antenn a ( FFO ) L o c a l os ci ll a t or 2 50-70 0 G H z

Description

Value
450 ­ 650 GHz 120 K 4 ­ 8 GHz < 1 MHz < 300 MHz < 30 mW < 4.5 K

Gas cell OCS measurements
· · · · Large discrepancy between modeled and measured spectra after first flights After thorough analysis strong nonlinearity in IF part of backend was found Possible saturation in IF chain resulted in power dependent line scaling of well-known OCS line. OCS gas cell measurements were performed to characterize nonlinearity effect for old data and to minimize it for 2011 flight measurements.

C o m puter c o nt r o l l e d da t a ac qu i s i t ion sy stem PL L S y n t he size r

H a rm o n i c S I S m i x e r fo r F F O p has e st a b il i z at io n (1 ) H E M T a m p lifie r (2 ) H E M T am pli f ie r I F am pli f ie r

I F am pli f ie r B a c k - e n d ( d ig ita l a u to c o rre l a to r)

Input frequency range Minimum noise temperature (DSB) Output IF range Spectral resolution LO frequency net Dissipated power at 4.2 K stage (including IF amplifiers chain 7 Operation temperature

Kiruna'2011 flight

Synoptic PSC areas over the last 20 years as compared to the present winter:

Calibrated OCS spectra, p=2.7mBar, FLO= 601.43 GHz.

· First launch with CNES team in Esrange · Exceptional geophysical conditions in the Arctic · First time recovery in Russia

Summary
Three successful flights of TELIS instrument in Kiruna (2009-2011) Remote operation of the SIR during all three flights Scientific observation program successfully completed Nonlinearity in IF part of the ACS was discovered Gas cell measurements were performed to characterize the instrument and correct the old data Data analysis of all three flights is now on-going Future aircraft, balloon and on-ground missions are under consideration
ISSTT 2011