Io-C and Io-D are radiated from the Jovian southern magnetic hemisphere and are generally left hand polarized.
Io-D is observed infrequently, it rarely reaches 20 MHz. Many of the modulations seen on the band of Io-D radiation are caused by the solar wind.
For 16 other Io-D related posts see:
http://herrero-radio-astronomy.blogspot.com/search/label/Io-D
For a method to use Jim Sky's wonderful Radio-Jupiter Pro 3 software to predict Io-D events see:
http://herrero-radio-astronomy.blogspot.com/2011/08/io-d-predictions-with-radio-jupiter-pro.html
http://www.radiosky.com/rjpro3ishere.htm
Many thanks to the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory, and Professor Imai Laboratory at Kochi National College of Technology in Japan
Io-D is observed infrequently, it rarely reaches 20 MHz. Many of the modulations seen on the band of Io-D radiation are caused by the solar wind.
For 16 other Io-D related posts see:
http://herrero-radio-astronomy.blogspot.com/search/label/Io-D
For a method to use Jim Sky's wonderful Radio-Jupiter Pro 3 software to predict Io-D events see:
http://herrero-radio-astronomy.blogspot.com/2011/08/io-d-predictions-with-radio-jupiter-pro.html
http://www.radiosky.com/rjpro3ishere.htm
Many thanks to the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory, and Professor Imai Laboratory at Kochi National College of Technology in Japan