Radio-Optical View of the Galaxy Hercules A - Many thanks to: NASA, ESA, S. Baum and C. O'Dea (RIT), R. Perley and W. Cotton (NRAO/AUI/NSF), and the Hubble Heritage Team (STScI/AURA)
Pulse at Parkes is an innovative project that provides high school students the opportunity to observe pulsars with the Parkes radio telescope, shown above. Click image for enlargement.
Muswellbrook High School observed on February 22.
Duncraig Senior High School Students and Faculty observing during a previous Pulse at Parkes session.
Pulsar J0437-4715 profile observed February 22 2010. This pulsar is part of the high priority Pulsar Timing Array project.
Map of the Io Phase versus the Jovian Central Meridian Longitude. This Map was coded by Junpei Azuma, Imai Laboratory, Kochi National College of Technology, Japan.
Detail above from the STEREO WAVES Behind spectrum near 10 UT.
Map of the Io Phase versus the Jovian Central Meridian Longitude. This Map was coded by Junpei Azuma, Imai Laboratory, Kochi National College of Technology, Japan.
Instrument pages: Helioseismic and Magnetic Imager, Stanford University 1 arcsecond resolution, full disk doppler velocity every 50 seconds 1 arcsecond resolution, full disk vector magnetic images every 90 seconds
Atmospheric Imaging Assembly, Lockheed Martin Solar Astrophysics Laboratory 1 arcsecond resolution images with multiple filters, every 10 seconds or better
The Radio Jove Archive shows entries for 24 days in 2007, from January to August. The Calendar above shows the 6 active days in April, one of the two most active months in the year.
John H. Thomas, W3FAF Radio Observatory, recorded an Io-C event on April 12. His Log notes he was using a 6 element tracking Yagi, with an Icom IC R75 receiver tuned to 20.92 MHz.