Data Usage Policy for Coordinated Jovian Radio Observations in 2016
Following the successful, initial coordination of Jovian S-burst observations in 2015 [1], we have extended coordinated Jovian radio observations with five powerful low-frequency radio telescopes in the United States, France, and Ukraine from 15 January to 4 May 2016. These observations were also a part of global Juno-supporting Jupiter observation campaign during its approach phase to the planet. These radio telescopes include the Long Wavelength Array station One (LWA1) in the United States, Nançay Decameter Array (NDA) in France, and three large radio telescopes (UTR2, URAN2, and URAN3) in Ukraine. For a full description of these data analyses see [2]. These data are accessible for the purpose of the collaborated research with other professional ground-based telescopes and amateur RadioJove telescopes in support of the Juno mission. Some of data are also accessible via Autoplot.
References
- Imai, M., A. Lecacheux, T. E. Clarke, C. A. Higgins, M. Panchenko, J. Dowell, K. Imai, A. I. Brazhenko, A. V. Frantsuzenko, and A. A. Konovalenko (2016), The Beaming Structures of Jupiter's Decametric Common S-bursts Observed from the LWA1, NDA, and URAN2 Radio Telescopes, Astrophys. J., 826, 176, doi:10.3847/0004-637X/826/2/176. [Erratum]
- Imai, M., A. Lecacheux, T. E. Clarke, C. A. Higgins, M. Panchenko, V. V. Zakharenko, A. I. Brazhenko, A. V. Frantsuzenko, O. N. Ivantyshin, A. A. Konovalenko, and V. V. Koshovyy (2019), Concurrent Jovian S-burst beaming as observed from LWA1, NDA, and Ukrainian radio telescopes, J. Geophys. Res. Space Physics, 124, 5302-5316, doi:10.1029/2018JA026445.
Collaborated research
The LWA1 Jupiter data used in this study were obtained through the following approved proposal.
Acknowledgements
We would like to thank the engineers and staff who operate the LWA1, NDA, UTR2, URAN2, and URAN3 radio telescopes. Construction of the LWA has been supported by the Office of Naval Research under Contract N00014-07-C-0147. Support for operations and continuing development of the LWA1 is provided by the National Science Foundation under grants AST-1139963 and AST-1139974 of the University Radio Observatory program.
Updated on August 29, 2019