Presentation is loading. Please wait.

Presentation is loading. Please wait.

SONGS OF JUPITER: DETECTING RADIO WAVES FROM SPACE Team 2

Similar presentations


Presentation on theme: "SONGS OF JUPITER: DETECTING RADIO WAVES FROM SPACE Team 2"— Presentation transcript:

1 SONGS OF JUPITER: DETECTING RADIO WAVES FROM SPACE Team 2
Tom Discepola, Greg Haislip, Shereef Elnahal, Mike Fitzsimmons, John Kang, Meera Krishnan, Saee Paliwal, David Paltiel, Henry Park, Margaret Senese Brian Holton Karl Strohmaier

2 Why is Jupiter Singing? 20 MHz radiation

3 Why is Jupiter Singing? 20 MHz radiation
First detected by Karl Jansky, 1928

4 Why is Jupiter Singing? 20 MHz radiation
First detected by Karl Jansky, 1928 Further research by Grote Reber

5 Why is Jupiter Singing? 20 MHz radiation
First detected by Karl Jansky, 1928 Further research by Grote Reber Source: Magnetosphere

6 Magnetospheres A magnetosphere is a large electromagnetic field that surrounds planets and other celestial bodies. Jupiter’s magnetosphere is larger than anything else in the solar system, including the sun.

7

8 Magnetosphere Jupiter’s Magnetosphere emits radio waves.

9 Magnetosphere Jupiter’s Magnetosphere emits radio waves.
Jupiter’s satellites create a ring of electrons, the torus.

10 Magnetosphere Jupiter’s Magnetosphere emits radio waves.
Jupiter’s satellites create a ring of electrons, the torus. A charged particle accelerating through a magnetic field will experience a force and emit electromagnetic radiation.

11 Solar Radio Emissions Type II solar emissions
Electron interference with solar winds.

12 Solar Radio Emissions Type II solar emissions
Electron interference with solar winds. Type III solar emissions Particle collisions in the solar wind cause radio wave emission. Solar flares release electromagnetic radiation across the spectrum. Solar bursts are caused by solar flares and emit radio waves close to 20 MHz.

13 Hypotheses 1. No signals 2. Just “noise” 3. Solar activitiy

14 Alternative Hypothesis that we have not fully REJECTED:
Little green mathematicians!!

15 Radio Telescope - Antenna
Function Intercepts radio waves and converts them to electrical current Designed to detect waves of frequency 20.1 MHz Explain WHY half the wavelength is necessary

16 Radio Telescope - Antenna
Construction Each dipole is approximately 7 meters, slightly less than λ/2. (λ = m)

17 Center Insulator

18

19

20

21 Problems Solutions Diodes Tuner SA602 chip Orient them correctly
Forget about it. Unfixable

22 Spend $300 and buy two receivers from Radio Shack.
ULTIMATE SOLUTION: Spend $300 and buy two receivers from Radio Shack.

23 Procedure Radio SkyPipe™ amplitude vs. time
Significance of two experiments

24 Data and Analysis Sharp peaks and hill-like lumps appeared on the graphs. Possible causes Sun Shortwave radio amateurs Storms Meteors Radio SkyPipe™

25 Data and Analysis Sharp peaks and hill-like lumps appeared on the graphs. Possible causes Sun Shortwave radio amateurs Storms Meteors

26 August 11, 2002, 8:34:07-13:28:59

27 August 11, 2002, 8:35:19-13:29:00

28 Conclusion Hypotheses confirmed Jupiter Solar emissions …and…

29 Surprise! Meteors!

30 and especially the one who makes us excited…
Acknowledgements State of New Jersey Drew University Brian Holton Dr. Miyamoto Dr. Surace taxpayers like you! and especially the one who makes us excited…

31 Oh yeah!


Download ppt "SONGS OF JUPITER: DETECTING RADIO WAVES FROM SPACE Team 2"

Similar presentations


Ads by Google