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Amateur Radio Astronomy (or “Another Way You Can Spend a Lot More Money in This Hobby”) By Don Pullen Presented to Cherry Springs Star Party – June 2012.

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Presentation on theme: "Amateur Radio Astronomy (or “Another Way You Can Spend a Lot More Money in This Hobby”) By Don Pullen Presented to Cherry Springs Star Party – June 2012."— Presentation transcript:

1 Amateur Radio Astronomy (or “Another Way You Can Spend a Lot More Money in This Hobby”) By Don Pullen Presented to Cherry Springs Star Party – June 2012

2 2 www.amateurastronomy.org

3 3 ?

4 What is Radio Astronomy? 4

5 5 What is Radio? Photons

6 Radio 6 Electromagnetic Spectrum (EM)

7 Science - Math 7 c = ƒ * λ or λ = c / ƒ or ƒ = c / λ E = h * ƒ Where: c = Speed of Light (~300,000,000 m/sec) λ = wavelength ƒ = frequency E = energy h = Planck’s constant (6.626 x 10 -34 Joules.sec)

8 Main points… 8 Radio, Light and more are all part of Electromagnetic spectrum separated by different frequencies and wavelengths. Frequency and wavelength are related. As frequency increases, wavelength decreases (and vice-versa). This means higher frequencies require smaller antennas. Higher frequencies means higher energy levels which results in different properties.

9 Radio Spectrum 9

10 Atmosphere 10

11 Atmosphere 11

12 Main points… 12 Only certain portions of the EM spectrum can reach the surface of the Earth since other portions are either reflected, refracted or absorbed by the Magnetosphere, the Ionosphere or the atmosphere. We know that the Ozone layer blocks most of the UV. Other components of the atmosphere also block other portions of the EM spectrum. To observe in other parts of the EM, we need satellites in space. Light reaches the Earth, as does most of the Radio EM and some Microwave and Infrared. This is why we use Radio and why it’s suitable for amateur work.

13 What can be seen? 13

14 What can be seen? 14

15 Radio Sources 15 Sun Jupiter Saturn & Venus (weak and intermittent) Center of Milky Way Pulsars Man-made sources

16 Amateur Radio Astronomy + 16

17 17 Amateur Radio Astronomy +

18 Radio Frequencies Used 18 Solar and Jupiter 13.36 - 13.41 MHz 25.55 - 25.67 MHz Pulsars 73.00 - 74.60 MHz 150.05 - 153.00 MHz 406.10 - 410.00 MHz Hydrogen Line Emission 1400.0 - 1427.0 MHz

19 Reserved Radio Frequencies 19

20 How to Get Started 20 CHEAT! Use the Internet

21 Amateur Radio Astronomy Organizations 21 SARA – Society for Amateur Radio Astronomers www.radio-astronomy.org NRAO – National Radio Astronomy Observatory www.nrao.edu AAVSO – American Association of Variable Star Observers www.aavso.org UKARANET – UK Amateur Radio Astronomers Network www.ukaranet.org.uk

22 Simplest - Meteor Detection 22

23 Meteor Detection Can use FM radio tuned to distant station – Best over 200 mi away – Use radio-locator.com for list of stations – Also wikipedia for stations by state FM normally is line-of-sight since escapes to space Ionization caused by meteor is reflective to various radio frequencies including FM. Independent of day/night cycle or solar activity. – But better after midnight when moving into meteors 23

24 Meteor Detection 24

25 Meteor Detection 25

26 Meteor Detection - Advanced 26

27 Solar Monitoring Cheat – use internet sites like SpaceWeather.com, or NOAA. 27 Other Solar Monitoring sites: SOHO – sohowww.nascom.nasa.gov SDO – sdo.gsfc.nasa.gov NSO – www.nso.edu Stanford – sun.stanford.edu

28 Solar - Indirect 28 Solar wind and energetic particles (X-Rays) constantly bombard Earth’s Magnetosphere and Ionosphere causing them to deflect or ionize.

29 Solar - Indirect 29 Changes in Ionosphere and Magnetosphere can be detected with 2 fairly simple techniques. Radio propagation Magnetometer

30 Solar - Indirect 30 Radio Propagation How radio signals “bounce” off the ionosphere

31 31 Solar - Indirect 31 Radio Propagation

32 Solar - Indirect 32 Radio Propagation

33 33 Solar - Indirect 33 Radio Propagation

34 34 Solar - Indirect 34 Radio Propagation

35 Solar - Indirect 35 SID – Sudden Ionospheric Disturbance Monitors a standard known radio signal and notes changes in signal strength directly indicating variations in ionosphere and indirectly indicating changes in solar X-Ray emission. Citizen Science!

36 36 Solar - Indirect 36 SID – Sudden Ionospheric Disturbance

37 37 SID – Receivers – Kits/Preassembled Solar - Indirect

38 38 Solar - Indirect SID – Antennas

39 39 Solar - Indirect SID – Antennas

40 40 Solar - Indirect SID – More Advanced

41 41 Solar - Indirect Magnetometer Monitors deflections in Earth’s magnetosphere by amplifying changes in compass bearings.

42 42 Solar - Indirect Magnetometer

43 43 Radio JOVE - radiojove.gsfc.nasa.gov Receiver Solar - Direct

44 44 Radio JOVE - Antenna Solar - Direct

45 45 Solar Bursts received near the frequency 20 MHz often turn on rapidly and decay slowly -- looking somewhat like a shark fin on the strip chart record. These bursts can be quite strong and often last for tens of seconds. You will hear the weak galactic background noise for several seconds, followed by a Solar radio noise burst. Radio JOVE - SOLAR BURSTS Solar - Direct

46 46 Jupiter L-Bursts sound like ocean waves breaking up on a beach. Much of the L-burst structure is formed as signals travel though the interplanetary medium from Jupiter to the Earth. Radio JOVE - JUPITER L-BURSTS Jupiter

47 47 Jupiter S-Bursts sound like a handful to pebbles thrown on a tin roof (or popcorn being cooked). These bursts each last for a few thousandths of a second and occur at rates as high as several dozen per second. Radio JOVE - JUPITER S-BURSTS Jupiter

48 Radio Jove - Advanced 48 Interferometry It’s possible to improve signal and reduce interference using a method called Interferometry. 2 or more stations/antenna systems are set up and data fed to computer to calculate similarities and differences.

49 Advanced 49

50 Advanced 50 IBT – Itty Bitty Telescope

51 Advanced 51

52 Advanced 52

53 Professional Radio Telescopes 53 NRAO – National Radio Astronomy Observatory www.nrao.edu (links to Greenbank, VLBA, ALMA & EVLA) Square Kilometer Array: www.skatelescope.org LOFAR – Low Frequency Array www.lofar.org Arecibo – www.naic.edu Deep Space Network deepspace.jpl.nasa.gov/dsn

54 Books 54 Radiosky publishing has a lot of books Radio Astronomy Projects by William Lonc ~$27 Radio Astronomy teachers Workbook ~$20 Radio Astronomy by John Kraus ~$50 Some others Radio Science Observing by Joe Carr – Prompt Publishing ~$70 An Introduction to Radio Astronomy by Bernard F Burke and Francis Graham-Smith – Cambridge University Press ~$80 (not a beginners book) The Radio Sky and How to Observe It by Jeff Lashley – Springer Publishing ~$30 Amateur Radio Astronomy by John Fielding – Radio Society of Great Britain ~$35

55 Miscellanea 55 List of Amateur Radio Astronomy websites: - www.bambi.net/sara/sites_list.html Good resource website: - radiosky.com Reserved Radio Frequencies for Astronomy - www.setileague.org/articles/protectd.htm - www.ukaranet.org.uk/basics/frequency_allocation.htm Pop Bottle Magnetometer - image.gsfc.nasa.gov/poetry/workbook/page9.html

56 References 56 www.radio-astronomy.org/pdf/sara-beginner-booklet.pdf www.nrao.edu/index.php/learn/radioastronomy www.cv.nrao.edu/course/astr534/ERA.shtml 1987 & 1999 ARRL Handbooks sid.stanford.edu en.wikipedia.org/wiki/Radio_astronomy www.aavso.org www.ukaranet.org.uk

57 Suppliers www.radioastronomysupplies.com www.alfaradio.ca www.thesatelliteshop.net 57

58 Thank You Presentation will be available online in about 1 week at: www.amateurastronomy.org under LINKS button


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