Abstract

Many undergraduate radio astronomy courses are unable to give a detailed treatment of aperture synthesis due to time constraints and limited math backgrounds of students. We have taken a laboratory-based approach to teaching radio interferometry using a set of college-level, table-top exercises. These are performed with the Very Small Radio Telescope (VSRT), an interferometer developed at the Haystack Observatory using satellite TV electronics as detectors and compact fluorescent light bulbs as microwave signal sources. The hands-on experience provided by the VSRT in these labs allows students to gain a conceptual understanding of radio interferometry and aperture synthesis without the rigorous mathematical background traditionally required. The data are quickly and easily processed using a user-friendly data analysis Java package, VSRTI_Plotter.jar. This software can also be used in the absence of the equipment as an interactive computer activity to demonstrate an interferometer’s responses to assorted surface brightness distributions. The students also gain some familiarity with Fourier transforms and an appreciation for the Fourier relations in interferometry using another Java package, the Tool for Interactive Fourier Transforms (TIFT). We have successfully used these tools in multiple offerings of our radio astronomy course at Union College

Highlights

  • We introduce here a set of labs at the undergraduate level which provide hands-on experience with the basics of aperture synthesis observations and how the data reveal information about the size and structure of the observed sources

  • These labs are designed to give students a conceptual understanding of aperture synthesis without the need for the dense mathematical formalism that usually accompanies the topic in graduate-level classes

  • We give a brief discussion of what an aperture synthesis observation entails, touching on only those aspects necessary to comprehend the principles demonstrated in these labs

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Summary

Introduction

Because of the complexity of the math involved, aperture synthesis is often excluded from undergraduate curricula in physics and astronomy. We introduce here a set of labs at the undergraduate level which provide hands-on experience with the basics of aperture synthesis observations and how the data reveal information about the size and structure of the observed sources. These labs are designed to give students a conceptual understanding of aperture synthesis without the need for the dense mathematical formalism that usually accompanies the topic in graduate-level classes

The basic concept of aperture synthesis
Equipment
Laboratory Exercises
The primary beam
A single resolved source
Double Sources
Mystery Source
Fourier Transform
Solar Diameter
Practical Experience in the Classroom
Concluding remarks
Full Text
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