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Radio Astronomy in School

Radio Astronomy in School. www.hardhack.org.au. Cezar Leşanu. Suceava “Ştefan cel Mare” State University Planetariu m / Observatory. Electromagnetic spectrum. Atmospheric electromagnetic opacity. www.wikipedia.com.

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Radio Astronomy in School

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  1. Radio Astronomy in School www.hardhack.org.au Cezar Leşanu Suceava “Ştefan cel Mare” State University Planetarium /Observatory

  2. Electromagnetic spectrum

  3. Atmospheric electromagnetic opacity www.wikipedia.com

  4. We highlight some radio astronomy projects promoted by renowned institutions around the Globe, relatively accessible in terms of level of knowledge required, availability of the equipment, and investment. These projects are addressed to high school and university students as well as to amateur astronomers, and involve the participants in a wide range of hands-on activities, from building, assembling, and calibrating the hardware setup to analyzing and sharing the data over the internet, all in a interdisciplinary learning process.

  5. Interactive NASA Space Physics Ionosphere Radio Experiments" • is a non-profit scientific, educational corporation, founded in 1989 by a team of NASA employees • investigation of very low frequency (VLF = 0 Hz to over 100 kHz) radio signals in the earth's magnetosphere • These signals are both manmade and naturally occurring (most of which originate from lightning)

  6. INSPIRE VLF3 receiver kit http://www.tnskynet.com Field observation setup: • INSPIRE VLF3 receiver with stereo cable • Portable cassette tape recorder with headphones • Whip antenna • Ground stake

  7. Links • INSPIRE project home page http://theinspireproject.org/ • “Listening to Northern Lights” Video http://www.youtube.com/watch?v=eHvdZdsIZxg • Live VLF Natural Radio Streaming http://abelian.org/vlf

  8. Radio Meteor Observation • meteoroids disintegrate at an altitude of 80 to 130 km • the trails they leave behind are full of ionized gases that reflect radio waves • distant VHF(30MHz-300MHz) radio signals can bounce off the meteor trail (forward scattering method) • can monitor meteor activity regardless the weather conditions and at daytime

  9. Radio detection of meteors Transmitter Continuous wave (FM carrier) Receiving station

  10. Radio Meteor Observation Experimental setup Black box FM radio receiver with digital frequency readout ( SSB receiver + PC interface + PC soundcard )

  11. Radio detection of meteors at “Nights of Perseids” festival,Horodnic 2008/2009.

  12. Radio Meteor Observatory On Line at USV

  13. Links • International Meteor Organization http://www.imo.net/radio • The G7IZU Radio Reflection Detection Page http://www.tvcomm.co.uk/radio/ • “Meteormania” Video – BBC 4 TV http://www.tvcomm.co.uk/radio/video/meteormania.wmv • Radio Meteor Observatory's On Line http://www.rmob.org/index.php

  14. is an education project to build and distribute inexpensive ionospheric monitors to students around the world • the monitors detect solar flares and other ionospheric disturbances • Earth's ionosphere reacts strongly to the intense x-ray and ultraviolet radiation released by the Sun during a solar event • the signal strength from a distant VLF transmitter, reflected by ionosphere, will follow this changes SID Sudden Ionosphere Disturbance monitor

  15. Super SID Receiver - simple and low-cost “wire-loop antenna” Super SID (New SDR based VLF receiver)

  16. Links • Stanford Space Weather Monitor program http://solar-center.stanford.edu/sid.html • Society of Amateur Radio Astronomers http://www.radio-astronomy.org/node/142 • Tennessee SkyNet Observatory http://www.tnskynet.com/SID-VLF.php

  17. NASA Radio Jove Project • was conceived in 1997 by a team headed by Jim Thieman at Goddard Space Flight Center • sold its first receiver kit 1999 (10th anniversary – almost 1400 kits sold) • observe and analyze natural radio emissions of Jupiter (bursts), the Sun (Solar flares), and our galaxy (transit)

  18. Frequency of operation 20.1 MHz • Receiver type: direct conversion (a hamradio transceiver can be used – expensive) • Antenna: dipol λ/2 or phased dipol or multi-element http://fringes.org/ phased dipole antenna

  19. Radio-SkyPipe Software - An Internet Enabled Strip Chart Recorder http://www.radiosky.com

  20. Radio Jove at ATLANTYKRON Summer Academy 200550th anniversary of the discovery of Jupiter's natural radio emissions

  21. Links • NASA Radio Jove Project http://radiojove.gsfc.nasa.gov/ • The Internet Jupiter Radio Observatory Kochi JP http://jupiter.kochi-ct.jp/ • Radio bursts from Jupiter video - CFARO http://www.youtube.com/watch?v=H6wkt_8a-6A • Radio burst from the Sun – CFARO http://www.youtube.com/watch?v=smuHQzDy3i0

  22. Small total power radio telescope Computer + data logging software Offset TV satellite dish Data acquisition board LNB Power Supply 14-18V DC Analog satellite finder (modified)

  23. Detect microwaves emitted by the Sun and approximate the temperature at 11GHz (chromosphere) • Detect microwaves emitted by the human body or any other object of sufficiently high temperature.

  24. First test - 2006 Meridian transit of the Sun at 11GHz (Ku band)

  25. Panaci 2009 Suceava Panetarium 2009

  26. The Internet Solar Radio ObservatoryImai Laboratory, Kochi National College of Technology, Japan http://sun.kochi-ct.jp/e/observatory.html

  27. Links • MIT Very Small Radio Telescope (VSRT)  http://www.haystack.mit.edu/edu/undergrad/VSRT/index.html • Radio Astronomy on 11 GHz at ISU http://astro.u-strasbg.fr/~koppen/10GHz/index.html • The Internet Solar Radio Observatory http://sun.kochi-ct.jp/e/observatory.html

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