Radio Astronomy Projects Table of Contents


Chapter 1: Some General Concepts

Overview of Possible Experiments		1 - 1

Right Ascension, Hour Angle, and Sidereal Time	1 - 4

Galactic Center at Meridian Crossing		1 - 10

Minimum Detectable Signal			1 - 12

Equivalent Blackbody Temperature		1 - 16

Calculating Receiver Bandwidth		1 - 22

Interferometer Symmetry			1 - 26

Angular Dependence of Fringe Spacing		1 - 31

Analyzing an Interferogram			1 - 35

Optimum Interferometer Spacing		1 - 37

A Benefit of Phase Switching		              1 - 40
  
Focal Point Heating			1 - 41

Square Law Detection			1 - 44

Phase Switched Interferometer		1 - 47

Finding the Local Meridian			1 - 49

Antenna Temperature			1 - 51


Chapter 2: Projects in the VHF and UHF Spectrum



Solar Disturbances at 265 and 435 MHz	2 - 1

Amateur Radio Telescope at 1296 MHz		2 - 3

Salvaged Mairsat Project			2 - 7


Chapter 3: Projects in the Microwave Spectrum



Beginner's Microwave Radio Telescope		3 - 1

4 GHz TVRO Telescope: Preliminary Observations	3 - 8

Very Small Radio Telescope at 4 GHz (Horn)	3 - 11

4 GHz TRF (Tuned Radio Frequency) Receiver	3 - 16

4 GHz Interferometer: 4m Baseline		3 - 21

4 Ghz Interferometer: 28m Baseline		3 - 24

Solar Radius at 4 GHz: 28m Baseline		3 - 26

Solar Radius at 4 GHz: 4m Baseline		3 - 28

Small 10 GHz Radio Telescope		3 - 31

The Moon at 11 GHz			3 - 34

Computerized Observations at 11 GHz		3 - 37

12 GHz Radio Telescope			3 - 41

Small 12 GHz Demonstration Radio Telescope	3 - 46

Back Yard Radio Astronomy		              3 - 49

Multi-antenna Radio Telescope		3 - 55

Home Built Pyramidal Horn Antenna		3 - 56

Home Built Waveguide to Coax Adapter	3 - 64

Spiral Antenna Feeds			3 - 67

Slot vs Spiral Antenna Feeds		              3 - 73
 

Chapter 4: Miscellaneous Projects


Second Detector: Crystal or Vacuum Diode?	4 - 1

Digitizer from an X-Y Recorder		4 - 4

Temperature Effects			4 - 8


Chapter 5: Signal Processing Concepts



Computer Simulated Signal Averaging		5 - 1

Signal Processing by Autocorrelation		5 - 4

Signal Processing by Multiplication		5 - 9

Fourier Transform: Why?			5 - 16

Fourier Analysis: How?			5 - 21

Fourier Synthesis: How?			5 - 27

Chapter 6: Student Research Papers


The Galactic Cenetr by Accident by Sherri Aker	                                          6 - 1

The Sun's Temperature at l = 5 cm   by Na Han Chan			6 - 3

Detecting the Galactic Center at 70 cm   by Jennifer Hatt			6 - 7

Interferogram Visibility Function for a 1/2 Degree  Source by S. W. Lee	6 - 12

Solar Temperature at 7.5 cm by George Lo	                                          6 - 15

Appendices:

A: Spectra of Major Observable Objects

B: Meridian Crossings at Local Standard Time

C: Sidereal Time at 0h Greenwich Mean Time

D: Sundial Corrections

E: Bibliography


Return to Radio-Sky Publishing home page.