PrimaLuceLab Radio2Space SPIDER 300A White Paper Download Page 6

WHITE PAPER

v2.1 (upd 09/10/2020)

EXAMPLES OF RESULTS WITH SPIDER radio telescopes 

SPIDER  radio  telescope  allows  you  to  make  radio  astronomy  studies  on  many  radio  sources  and  to 
record  different  types  of  results  as 

transits,

 

spectra

  and 

radio-maps

.  Here  you  find  a  few  examples  of 

studies recorded with SPIDER radio telescope. 
 

Taurus A radio map: 

Taurus A is the radio source in

 

Taurus

 

constellation that corresponds to 

the  Crab  Nebula  (M1),  the

 

supernova  remnant  exploded  on  July  4, 

1054 and noted by Chinese and Arabian

 

astronomers of the time. A 

radio telescope is different from an optical telescope by many aspects: 
one of these is that it collects radio waves from a single area in the 
sky.  Just  to  give  an  example,  it's  like  having  a  telescope  with  a  CCD 
camera that comes with a single large pixel. In order to create radio 
maps,

 

technique

 

consists  in  moving  the  antenna  with  small 

movements  and,  for  every  sky  position,  record  radio  waves  coming 
from  space

 

tracking  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 captured and displays this value with a color based 
on a color scale chosen by the user. RadioUniversePRO software allows you to point the radio telescope 
to  the  precise  sky  position  of  the  radio  source,  visualize  in  real  time  the  bandwidth  spectrum  in 
frequency  so  you  can  see  if  you  have  artificial  signal  in  it  (allowing  you  to  filter  these  from  your 
recordings) and define radio map specifications.  

With a 3 hours capture time, setting the following 
parameters in RadioUniversePRO: 

Map dimensions: 15 x 15

 

degrees 

Pixel separation: 0,4

 

degrees 

Integration time for every pixel: 5 seconds 

The result is the map that we

 

show in the image. 

You  can  easily  see  the  increase  of  the  signal  at 
the center of the map, corresponding to Taurus A 
position. The increase in the visible signal at the 
top  right  of  the  image  is  the  Milky  Way,  in  fact 
Taurus A does not lie perfectly on the plane of our 
galaxy but it is a few degrees away (as confirmed 
by the radio map). 

pag. 6

Summary of Contents for Radio2Space SPIDER 300A

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

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

Page 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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