Radio Astronomy (ASTR700), Spring 2020
[SPRING 2022 STUDENTS: your course materials are on https://ecampus.wvu.edu/]
Live course schedule (revised for online course).
Student-led lecture rubric
Here is a radio view of Hydra A using different configurations of the Very Large Array, whose A (biggest) to D (most compact) arrays provide different resolutions, and change the telescope's sensitivity to differing scales of emission.
Student-led lecture rubric
Lecture materials---
slides, links, and assess-yourself activities:
Tues January 14: Introduction
[ Slides ]
[ Self-review ]
Thurs January 16: Quantifying Light
[No slides today]
[ Self-review ]
Tues January 21: [ problem solving session #1 ]
Thurs January 23: Blackbodies and Accelerated Charges
[No slides today]
[ Acceleration geometry figures ]
[ Link: Interacting with accelerated charges ]
[ Self-review ]
Tues January 14: Introduction
[ Slides ]
[ Self-review ]
Thurs January 16: Quantifying Light
[No slides today]
[ Self-review ]
Tues January 21: [ problem solving session #1 ]
Thurs January 23: Blackbodies and Accelerated Charges
[No slides today]
[ Acceleration geometry figures ]
[ Link: Interacting with accelerated charges ]
[ Self-review ]
Tues January 28: Fourier Transforms & Friends
[ Slides ]
Thurs January 30: [ problem solving session #2 ]
Thurs February 13: [ problem solving session #3 ]
[ Slides ]
Thurs January 30: [ problem solving session #2 ]
Thurs February 13: [ problem solving session #3 ]
Tues February 18: Radiometers
[ Parkes multibeam receiver parameters shown in class ]
[ Very Large Array receiver parameters shown in class ]
[ Parkes multibeam receiver parameters shown in class ]
[ Very Large Array receiver parameters shown in class ]
Thurs February 20: Interferometry
[ Slides ]
[ Standard thorough reference text for interferometry ]
[ Quick-read reference for intererometery ]
Tues February 25: [ problem solving session #4, including solutions ]
Tues March 3: Emission Mechanisms Overview and HII Regions
[ Continuum emission Quick-ref ]
[ Notes ]
[ Slides ]
[ Standard thorough reference text for interferometry ]
[ Quick-read reference for intererometery ]
Tues February 25: [ problem solving session #4, including solutions ]
Tues March 3: Emission Mechanisms Overview and HII Regions
[ Continuum emission Quick-ref ]
[ Notes ]
Thurs March 5: Thermal Bremsstrahlung
[ Project introduction notes ]
[ Notes ]
Tues March 10: Magneto Bremsstrahlung
[ Slides ]
Thurs March 12: Synchrotron Spectra & Sources [Will & Jacob student lecture]
[ Will & Jacob student lecture slides ]
Tues March 31: [ problem solving session #5, including solutions ]
[ Project introduction notes ]
[ Notes ]
Tues March 10: Magneto Bremsstrahlung
[ Slides ]
Thurs March 12: Synchrotron Spectra & Sources [Will & Jacob student lecture]
[ Will & Jacob student lecture slides ]
Tues March 31: [ problem solving session #5, including solutions ]
Tues April 7: Pulsars
[ Elaine slides ]
[ Evan slides ]
Thurs April 9: Fast Radio Bursts, ISM concepts, and Source counts
[ Slides ]
Tues April 14: [problem solving session #6]
[ Slides and project ideas ]
Thurs April 16: Recombination lines [Jess & Dylan student lecture]
[ Slides ]
[ Bohr atom simulation link ]
[ Elaine slides ]
[ Evan slides ]
Thurs April 9: Fast Radio Bursts, ISM concepts, and Source counts
[ Slides ]
Tues April 14: [problem solving session #6]
[ Slides and project ideas ]
Thurs April 16: Recombination lines [Jess & Dylan student lecture]
[ Slides ]
[ Bohr atom simulation link ]
Here is a radio view of Hydra A using different configurations of the Very Large Array, whose A (biggest) to D (most compact) arrays provide different resolutions, and change the telescope's sensitivity to differing scales of emission.
