Jupiter 140626, hectometric radiation with attenuation lanes, Sun 140628, hour long type VI with positive frequency drift

Many thanks to Dr. Baptiste Cecconi for his analysis of Jovian hectometric radiation (HOM) with attenuation lanes in STEREO WAVES B 140626.



Many thanks to the Taxpayers of France, and the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory.

The vertical scale is hours and minutes of Universal Time
The horizontal scale is MHz
The dynamic range from black to white is 20 decibel

Sun 140627, types I III V

Many thanks to the Taxpayers of France, and the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory.

The vertical scale is hours and minutes of Universal Time
The horizontal scale is MHz
The dynamic range from black to white is 30 decibel

Sun Jupiter Earth 2014 June

Many thanks to the STEREO and WIND WAVES Teams

The vertical scale is log MHz
The horizontal scale is hours of Universal Time
The color visualization is relative

 

Sun 140623, type II with fundamental and second harmonic, type III

Many thanks to the Taxpayers of France, and the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory.

The vertical scale is hours and minutes of Universal Time
The horizontal scale is MHz
The dynamic range from black to white is 15 decibel

Jupiter 140616, Io-D at STEREO WAVES B

Many thanks to the STEREO WAVES Team and Prof. Dr. Kazumasa Imai, Kochi National College of Technology, Kochi Japan.

The vertical scale is log MHz
The horizontal scale is hours of Universal Time
The color visualization is relative

Sun 140612, type II at WIND WAVES, Sun 140617, types III V VI

Many thanks to the Taxpayers of France, the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory, Trinity College Dublin Ireland Astrophysics Group, NOAA SWPC, NASA SDO HMI Magnetograph Team, and WIND WAVES Team.

Below WIND WAVES 140612

Below
The vertical scale is hours and minutes of Universal Time
The horizontal scale is MHz
The dynamic range from black to white is 30 decibel

Poland will build 3 LOFAR stations

http://www.astron.nl/about-astron/press-public/news/three-new-antenna-stations-lofar-poland/three-new-antenna-stations-lo

"...ASTRON and the Polish LOFAR consortium POLFAR signed a contract for the construction of three new antenna stations for the International LOFAR Telescope (ILT) in the north, west and south of Poland. Signing of the contract took place at the University of Warmia and Mazury in Olsztyn in Poland in the presence of representatives of ASTRON, the Polish Ministry of Science and Higher Education and local governments, and representatives of the Polish astronomical and space sciences communities..."

"...At the end of 2013, POLFAR received a grant from the Polish Minister of Science and Higher Education for the construction and equipment of three international LOFAR stations as part of their national research infrastructure investment. The new LOFAR stations will be located in Łazy (in southern Poland, operated by the Jagiellonian University in Krakow), Bałdy (in northern Poland, operated by the University of Warmia and Mazury in Olsztyn), and Borówiec (in western Poland, operated by the Space Research Centre of the Polish Academy of Sciences). The formal agreement between the POLFAR consortium and ASTRON now marks the start of the preparations for the roll-out of these new stations..."


  
Above:
"...representatives of POLFAR and ASTRON at the LOFAR signing ceremony: Prof. Jerzy Jaroszewski (Vice Rector for Research of University of Warmia and Mazury), Prof. Andrzey Krankowski (University of Warmia and Mazury), Prof. Katarzyna Otmianowska-Mazur (coordinator of POLFAR, Astronomical Observatory of the Jagiellonian University), Dr. Marian Soida (Vice Director of the Astronomical Observatory of the Jagiellonian University in Kraków), Ronald Halfwerk (Director of AstroTec Holding, ASTRON), Ass. Prof. Hanna Rothkaehl (Space Research Center of Polish Academy of Sciences in Warszawa), Rene Vermeulen (Director of the ILT, ASTRON), Dr. Krzysztof Chyży (Astronomical Observatory of the Jagiellonian University) and Ass. Prof. Ewa Szuszkiewicz (Head of the Institute of Astronomy and Astrophysics of the Szczecin University)..."

Sun 140610, east limb pair of X2.2 and X1.5 X-ray flares, radio emission of types II IV V reaching over 40 decibel above background

Many thanks to the Taxpayers of France, the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory, NOAA SWPC, NASA SDO, and Lockheed Martin Solar Laboratory.

The vertical scale is hours and minutes of Universal Time
The horizontal scale is MHz
The dynamic range from black to white is 40 decibel

Sun 140606, 6 selected spectra, types II (fundamental and second harmonic) III V VI

Many thanks to the Taxpayers of France, the Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory, Trinity College Dublin Ireland Astrophysics Group, NOAA SWPC, and NASA SDO HMI Magnetograph Team.

The vertical scale is hours and minutes of Universal Time
The horizontal scale is MHz
The dynamic range from black to white is 20 decibel in 5 spectra below

 The dynamic range from black to white is 30 decibel below