Abridged Technical Description of the EISCAT Svalbard Radar


The EISCAT Svalbard Radar - the ESR - is a high power UHF radar to be operated near Longyearbyen, which is the main community on the island of Spitsbergen belonging to the archipelago of Svalbard. The funding, planning, construction and operation is performed as an integral component of the EISCAT Scientific Association. The radar system is designed to allow incoherent scatter observations of the iono,sphere and extendable for coherent scatter observations of the middle and lower atmosphere. Detailed full system specifications of the EISCAT Svalbard Radar was compiled for release in the Baseline Description Document. A summary follows here:

INFRASTRUCTURE:

Location: 12 km south-east of Longyearbyen at 78 09'N, 16 02'E and 434 m above MSL, about 550 m south of the main entry to Mine 7 of the Store Norske Mining Company

Road Access: Open road from Longyearbyen to Mine 7 and extension road to the radar

Electrical power: 22 kV line serving Mine 7, step-down transformers, emergency generator on site

Building: Operations building close to the antenna, consisting of transmitter hall, instrument and control rooms as well as office, workshop, laboratory, storage and personnel facilities rooms. Fully shielded for minimum radio frequency interference and electromagnetic compatibility. Constructed for severe Arctic climate conditions.

INSTRUMENTATION:

The initial configuration will consist of one parabolic dish antenna and a 500 kW peak power transmitter with 125 kW average power. The operating frequency will be close to 500 MHz. The receiver, data acquisition and analysis will apply state-of-the art digital signal processing standards and devices. This configuration wresult in a system sensitivity , which is about equal to the present monostatic EISCAT UHF radar in Tromsø.

Frequency:	Centre:		500 MHz
		Bandwidth:	±2 MHz (transmit)
				±10 MHz (receive)

Antenna(s) specifications:

Type: Circular parabolic dish of 32 m diameter design with solid surface. Slewing ring (turning head) type, designed for severe Arctic climate conditions:

Temperature range:		-55  ÷ +25 C
Operational wind speed:		less than 27 ms-1
Survival wind speed:		50 ms-1
Ice warning system

Slewing rate (elev. + azim.):	1.5  s-1
Slewing acceleration:		1  s-2
Slewing range:			elev.:	0  - 180 
				azim.:	± 270 
Pointing accuracy:		less than 0.05

Feed system:	 		Secondary focus,
				waveguide, 2 rotary joints
Polarization: 			Circular (right-hand transm. 
					  left-hand receive)

Gain:			 	42 dBi
Sidelobes:			-16 dB (1. sidelobe)
				-24 dB (2. sidelobe)
				-34 dB (3.-5. sidelobes)
				less than -40 dB (others)
VSWR:				less than 1.20

Ant. temperature:		45 K at 90  elevation
(Sky-, preamp. noise etc.)	60 K at 10  elevation
Max. power:			2 MW peak, 500 kW average

Transmitter:

Type: Modular system consisting of combined single RF-amplifier modules, which allows high redundancy, use of standard amplifiers and easy system expansion to higher power levels.

The single modules base on standard television transmitters employing external cavity vapor cooled klystron tubes yielding 62.5 kW RF-power. A beam pulse modulator is added.

The transmitter is being constructed by Harris Allied Broadcast Division, Cambridge, UK (delivery for tests in Tromsø in summer 1993). The klystron tubes will be supplied by 2 independent vendors, Philips, Germany, and EEV, UK. These klystrons have typical lifetimes of about 25000 hours.

Module 1 (prototype):

Power:				250 kW peak
			  	obtained by combining 4x62.5 kW
Power bandwidth (-1dB):	4 MHz
Duty cycle:			25 % max.
Input power:			10 mW
Load VSWR:			less than 1.2
Harmonic emission:		-60 dBc
Spurious emission:		-50 dBc
Interpulse noise:	   	less than -155 dBm/Hz
Pulse length:			1 µs ÷ 2 ms
Rise/fall time:			less than 0.5 µs
Voltage droop (at 2ms):	3 %
Pulse rep. rate:		0.02-2 kHz
Interpulse period:		0.5 ms min.
Modulation:			amplitude and phase
Dynamic range:			20 dB
Mains voltage:		   	3-phase 400 V
HV for klystron:	   	23-27 kV
Power combiner (2x125 kW):	switchless
Harmonic filter
Security:			Obey standards on RF leakage, magnetic 
				and electric fields, x-ray and materials
Control and monitor:		allow mostly unattended operation
				under automatic or remote control
Cooling:			air and water vapor
Size (lxwxh):			5.2 x 4.2 x 3.1 m
Klystrons:			YK1265, EEV K3673BCD

Module 2:

Same as module 1. To be ordered in 1993 when module 1 has been tested. Modules 1 and 2 will subsequently be combined on Svalbard to yield the peak RF-power level of 2 x 250 kW = 500 kW. In later expansion phases further modules can be added.

Radar Controller:

The radar controller is a dual design. One controller is in control while the other is accessible from the crate CPU. The idea is to be able to reload the radar controller program during operation. If it is possible to fit two radar controllers on one VME card, this solution is to be preferred.

Inputs: A 10 MHz clock signal (sinus), a 100 Hz synchronization pulse and a start command from the real time clock.

Program memory: The address space is 20 bits. This means that it may contain up to 1 M Word memory. This gives the maximum program size that will be possible with this design. How much memory that actually will be instal will depend on how much memory we can fit on a VME card in addition to the other circuits. The aim is to install at least 256 k word on the prototype.

The memory is organized so that each word contains a 32 bit control word section, a 24 bit dwell time section and 8 bits for internal control and program instructions. Outputs: 32 bit control word with 100 nanoseconds time resolution, 1 bit end of scan.

Receiver:

The receiver chain is configured as a dual superheterodyne with a first IF at 70 MHz and a second IF at 7.5 MHz or higher. This is sampled at 10 MHz at 12 bits of resolution. All further frequency translation, filtering, rate decimation and/or resampling is performed in a digital back end before the data stream passes into the digital signal processing units. The receiver is fully phase coherent, i.e. all oscillators, including the sampling clocks, are phase locked to, or derived from, a common reference.

The three main subsystems of the receiver are:

(a) Front-end: low noise cooled GaAsFET preamplifier and high dynamic range first mixer. Physically located in the antenna cabin. Equipped with low noise local oscillators.

Flange noise temperature:		less than 20 K
Bandwidth (- 3dB):			60 MHz
Overall gain:				40 dB
Local oscillator step size:		2 (1) MHz
Output band (each mixer):		70 ±5 MHz

There can be up to three, first mixers connected to the common preamplifier, each with its own local oscillator and its own IF distribution and back end.

(b) IF distribution: first I.F. stages and the second mixer(s). Physically located at a central point in the RF equipment area (possibly the transmitter hall). One independent IF distribution subsystem for each first mixer output from the front end.

Input band:				70 ±5 MHz
Number of outputs:			up to 4
Output ban				7.5 ±2 MHz
    					or 5.0 ±4 MHz
2nd LO frequency:			77.5 MHz, 75 MHz
(individually selectable for each mixer/output)
Total gain:				>130 dB
Output level:				2 V pk-pk into 50 ohms

(c) Back-end: sampler, A/D converter, complex digital mixer and FIR filters. These will be realized in all digital technology. One independent back end for each IF distribution channel output. More than one mixer and FIR filter can be connected to the same ADC over a broadcast mode data bus.

Receiver back end specifications:

Bus environment:			VME
Analog-Digital-Converter:
Input power bandwidth (-3 dB):   	25 MHz min.
Sample rate (sustained):		10 MHz min.
Resolution:				12 bits min.
Input voltage for 1 MSB:		1.024 V
Input impedance:			50 + j0 *
Digital multiplier:
Input bandwidth:			10 Mhz min.
Frequency resolution:			less than 0.01 Hz

HW FIR filter:
Input data rate:			10 MHz min.
Number of taps:				512 min.
Coefficient accuracy.			16 bits min.
Decimation:				2,..., 512 min.

Digital Signal Processors (DSP):

These should be of two types, viz. devices optimized for narrowband modes and lagprofile computations, using industry-standard DSP-specific microprocessors, and devices optimized for wideband modes and/or fast decoding, using special-purpose FFT processor hardware. Initially, only the narrowband mode devices will be implemented. Commercially available VME-compatible boards are used to configure the system.

DSP specifications:

Bus environment:			VME
Host processor type:			SparcEngine 2 or 68040
Lag profile processor:			Chip family TMS 'C40
Input data rate/processor:		10 MHz max.
Input data format:			16+16 bit complex
Output data format:			32+32 bit complex
 					or IEEE FP
Processing rate (complex mpy/add):	30 MOPS/channel

Computing, Software

Theucture of the software systems will be as follows:

The software will be divided into two main areas which will communicate via a data base system. The first area:

(a) will contain all the time-critical elements, while the second,
(b) will contain all the packages required to use the radar for scientific purposes.

The two areas will provide a logical separation between (a) the real-time tasks and (b) the user packages. A further series of interfaces to the database system will provide engineering information both for operational maintenance and long term monitoring.

The design philosophy behind the EISCAT Svalbard Radar system procurement exercise is to use high-technology industry-standard components and subsystems wherever possible. In-house design is tried to be kept at minimum, although the expertise of inhouse staff, acquired over many years of the EISCAT operation, is indispensable in defining, supervising and developing certain system partitions of the hardware and software. This is mandatory to allow a system design and development, which is exceptionally specialized as an advanced incoherent and coherent scatter radar system. Associates' institutions support on certain work packages, such as software design is also envisaged.

The design of the industry-constructed system parts will be in close coordination with experienced EISCAT staff and selected consultants from other observatories and Associates' institutions. The testing of many parts will be performed at the mainland sites before these will be installed on the site near Longyearbyen in 1994 and thereafter. Test operation is planned to start at the end of 1995, experiments should commence as soon as possible after successful testing. Later remote monitoring and control from an operations centre in the Longyearbyen community or at the land is planned to be added, when corresponding facilities and funds will be available.


Document : ANRE92A.DOC (part)

Created : 6.11.93

By : Jürgen Röttger

HTML debugged and edited 02/08-95 by Bjørge; Brekke