THIS MEETING HAS BEEN CANCELLED DUE TO WEATHER
We will reschedule Dr. Locke to speak at a future meeting.
February 8, 2017, 7:30PM, University of Victoria, Bob Wright Centre A104 – RASC Victoria Centre’s monthly meeting
Radio and Microwave Astronomy – History, Canadian Involvement, and Interesting Tidbits – Dr. Lisa Locke, NRC Herzberg
Radio astronomy started in the early 1930s as an electrical engineering project and it took many years for the optical astronomy community to include it under the gilded Astronomy umbrella. Early experimentalists had a field day with surplus World War II equipment and the increased world-wide collaboration between researchers. I will explain and guide through this history up to the present, contrasting the new radio astronomy with the classic well-understood optical ideas, highlighting Canada’s significant role in the growing field. Details on current instrumentation projects and observatories will also be presented.
Dr. Lisa Shannon Locke was born north of the 60th parallel in Hay River, Northwest Territories, Canada and received the B.Sc (Alberta, 1997), M.Sc. (Cape Town, 2001) and PhD (Victoria, 2014) degrees all in electrical engineering specializing in low-noise microwave astronomy instrumentation.
As a student, she worked at the Canadian Space Agency, CalTech’s Owens Valley Observatory and at the National Radio Astronomy Observatory in Green Bank, WV. After graduating, she spent five years as a receiver engineer at the Arecibo Observatory in Puerto Rico. Then in 2005 she joined the National Radio Astronomy Observatory, Socorro, NM building cryogenic receivers for the expanded very large array (EVLA).
Her PhD degree was advised by Prof. Dr. Jens Bornemann and the late Dr. Stéphane Claude of NRC Herzberg Institute of Astrophysics, Victoria, BC. Her thesis investigated the design and construction of a K-band (18 – 26 GHz) coherent 5×5 phased array feed for use on large radio astronomy reflectors. She is currently employed with NRC Herzberg and leads a multi-disciplinary project to build a S/C-band (2.8 – 5.18 GHz) cryogenic phased array feed receiver system.