PrimaLuceLab Radio2Space SPIDER 300A Скачать руководство пользователя страница 13

WHITE PAPER

v2.1 (upd 09/10/2020)

ENVIRONMENTAL CONDITIONS 

The SPIDER 300A is designed for mount and antenna installation outside. The environmental conditions 
to be met for proper operation are: 

The receiver of the SPIDER 300A radio telescope is installed inside, in a control room specially protected 
by  environmental  phenomena  (rain,  snow,  hail).  It  is  preferable  to  install  the  receiver  in  a  room  with 
temperature as constant as possible. 

Wind speed is one of the most important parameters to consider for the safe use of the radio telescope 
installed outside. SPIDER 300A radio telescope is safe for installation in external environments and does 
not require coverage. For safe use, you have to: 

• When  not  in  use,  the  SPIDER  300A  radio  telescope  is  to  be  placed  in  the  stow  position  with  the 

antenna pointing to the vertical (Zenith). In this way the antenna offers the minimum wind resistance.  

• When in use, the SPIDER 300A radio telescope is designed for operations with winds up to 50 Km/h 

(30 Mph). When the wind speed is higher, place the SPIDER 300A radio telescope in Stow Position and, 
if  necessary,  lock  the  antenna  with  the  stop  rod.  The  UltraSonic  Wind  Sensor  for  SPIDER  radio 
telescopes  (optional)  allows  you  to  constantly  monitor  the  wind,  using  the  RadioUniversePRO 
software provided with the radio telescope. This will automatically move the SPIDER 300A to stow 
position when the wind exceeds the 50 Km/h (30 Mph) safety threshold. 

Condition

Temperature

from -10 °C / 14 °F to +50 °C / 122 °F 

Maximum wind speed during use

50 Km/h (30 mph)

Maximum wind speed in stow position

150 Km/h (90 mph)

pag. 13

ATTENTION:

 because of unpredictable natural events that are not covered by the warranty, if the wind 

is  too  high  we  designed  a  “safe  release”  mechanism  that  disconnect  the  mesh  material  from  the 
antenna  body  and  save  the  rest  of  the  radio  telescope.  This  way  you  can  change  only  part  of  the 
antenna damaged by the wind with a new element of the antenna (that you can request to us as spare 
part).

Extended temperature version:

 For operation in extreme temperature conditions (lower or higher than 

the above table condition), a version of SPIDER 300A specially designed mount is to be required and 
specifically requested by the customer prior of the order.

Содержание Radio2Space SPIDER 300A

Страница 1: ...d 09 10 2020 Radio2Space is a brand of PrimaLuceLab iSrl via Roveredo 20 b 33170 Pordenone Italy All rights reserved reproduction prohibited even partial Information and conditions subject to change w...

Страница 2: ...parabolic antenna on the mount avoiding bending and ensuring the effectiveness of the pointing system They also help to maintain a perfect parabolic shape with a maximum error of less than lambda 20 F...

Страница 3: ...ecial electronic security system which parks the antenna pointing the Zenith the vertical position when the wind exceeds 50 Km h so that the radio telescope moves and is safety locked in the position...

Страница 4: ...e Universe Software SPIDER 300A comes with RadioUniversePRO the first software specifically designed to allow everyone get professional level radio astronomy results but in easy way The software allow...

Страница 5: ...real time the received band with FFT BBC Tools it allows you to identify artificial interferences and cancel them from recorded data Offset alignment automatic mount alignment on radio sources Source...

Страница 6: ...acking the sky apparent movement Then the SPIDER antenna is moved to a new position and record the next pixel value For every pixel RadioUniversePRO software calculates the total amount of radio waves...

Страница 7: ...ossible to record radio signals coming also from objects outside the Solar System Then we used the advanced features of SPIDER and RadioUniversePRO software to record the incoming signal from Cassiope...

Страница 8: ...every part may weight up to 150 kg and be as long as 3 meters Ladder at least 2 meter high Meter Cutter Soldering iron and solder wire Hot air gun Screwdrivers set Caliber Nipper Extension cord 17mm 1...

Страница 9: ...en the control room internal and the radio telescope external Check for soil characteristics geological parameters and planarity Keep in mind the size and weight of the machine Verify that the environ...

Страница 10: ...at has to be dimensioned based on the legislation of the country of installation One grounding will be closed to the pier base and one grounding will be in the control room to connect the surge protec...

Страница 11: ...ecially for soil characteristics you can show the professional the Installation site section and the foundation scheme installation scheme In this section you will find the scheme of foundation to be...

Страница 12: ...E SCALA TT 10 000 07 SPIDER 300A FOUNDATION 1 DI 1 O C PESO Kg MOD DESCRIZIONE DISEGNATO DATA APPR CODICE DATA A2 21 02 2017 FOGLIO TOLLERANCES ARE TO BE ACCORDING TO UNI EN 22768 1 UNLESS OTHERWISE S...

Страница 13: ...igher place the SPIDER 300A radio telescope in Stow Position and if necessary lock the antenna with the stop rod The UltraSonic Wind Sensor for SPIDER radio telescopes optional allows you to constantl...

Страница 14: ...olutely defined by the supplier of the UPS Lightning protection Due to the possible emission of radio waves and therefore the creation of strong interference a lightning arrestor system can not be ins...

Страница 15: ...be carried out as required by the relevant provisions The radio telescope must be installed on a concrete plinth that must conform to the plans provided by PrimaLuceLab The concrete plinth must be pr...

Страница 16: ...y suggest lower distances To allow proper antenna handling each coaxial cable is made up of 2 parts n 2 Ecoflex 10 coaxial cables that connect LNAs to the cables in the channel n 2 Ecoflex 10 coaxial...

Страница 17: ...WHITE PAPER v2 1 upd 09 10 2020 RADIO TELESCOPE AND CONTROL ROOM CONNECTIONS pag 17...

Страница 18: ...Aluminum Gain 0 0009 K Jy Polarization circular double Central frequency 1420 MHz Receiver band 50 MHz Noise temperature 50 K Channels number 1024 A D converter 14 bits Elevation range 0 90 Azimuth ra...

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