Introduction To Solar Weather : 10AM-11AM : Austin Room

 Lewis Thompson W5IFQsolarwx

 High Frequency Radio propagation is dependent on Solar Weather. Ultraviolet radiation from the sun creates and maintains the ionosphere.

Solar flares, coronal mass ejections and coronal holes, also from the sun can deteriorate or disrupt HF propagation.    This presentation will introduce the positive and negative effects of solar weather  on HF
propagation, and how the radio amateur can detect and compensate for these effects and maintain HF communications.

 

 

 Lewis Thompson W5IFQ

W5IFQLewis Thompson is a Senior Engineering Scientist (mostly retired) for Applied Research Laboratories, University of Texas at Austin. During his 44 years of employment, he worked the areas of underwater acoustics, and radio communications. His has been a licensed amateur radio operator since 1961 and is now licensed Extra Class. He held amateur radio leadership positions including President of the Austin Amateur Radio Club, RACES District Radio Operator (DRO-62) and Assistant Emergency Coordinator for TCARES. He joined Texas Army MARS in 2006 and served as State MARS Director from 2009 to 2011.   He is a Warrant Officer 1 in the MARS Detachment of the Texas State Guard and currently is the Special Consultant to the Texas Military Forces for Texas Army MARS.