Titles of some Juno related papers submitted to Geophysical Research Letters

Selected from :

http://www-pw.physics.uiowa.edu/plasma-wave/juno/publications.html

Direction Finding Measurements of Jovian Broadband and Narrowband Kilometric Radiation From the Juno Waves Instrument Near Perijove 1

Latitudinal Beaming of Jovian Decametric Radio Emissions as Viewed From Juno and the Nançay Decameter Array

A New View of Jupiter's Auroral Radio Spectrum

Generation of the jovian hectometric radiation: first lessons from Juno

Electron butterfly distributions at particular magnetic latitudes observed during Juno’s perijove pass

Io-Jupiter decametric arcs observed by Juno/Waves compared to ExPRES simulations

Plasma waves in Jupiter's high latitude regions: Observations from the Juno spacecraft

Statistical study of latitudinal beaming of Jupiter's decametric radio emissions using Juno

Electron beams and loss cones in the auroral regions of Jupiter

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Introductory Radio Astronomy references
http://herrero-radio-astronomy.blogspot.com/2015/06/introductory-radio-astronomy-references.html?m=1
Jupiter events at STEREO A for correlation with Juno Waves
http://herrero-radio-astronomy.blogspot.com/2016/12/jupiter-events-at-stereo-for.html
Links to Juno related posts
http://herrero-radio-astronomy.blogspot.com/2016/01/links-to-juno-related-posts.html?m=1
Sun Earth Jupiter event posts:
http://herrero-radio-astronomy.blogspot.com/2017/02/sun-earth-jupiter-20170223.html
http://herrero-radio-astronomy.blogspot.com/2015/08/links-to-monthly-sun-earth-jupiter-posts.html?m=1
Solar Cycle 24
https://en.wikipedia.org/wiki/Solar_cycle_24
"The Solar Cycle" by David Hathaway 2015, 81 pages
http://arxiv.org/pdf/1502.07020v1
Driel-Gesztelyi and Green 2015 "Evolution of Active Regions" 98 pages, 11 MB:
http://link.springer.com/content/pdf/10.1007%2Flrsp-2015-1.pdf
Links to recent Solar Radio Science Highlights by Eduard Kontar
http://herrero-radio-astronomy.blogspot.com/2017/02/links-to-recent-solar-radio-science.html
Solar Type Examples
http://herrero-radio-astronomy.blogspot.com/2015/07/solar-type-examples.html
Solar Dynamics Observatory - Now and Daily - Images Movies
http://sdo.gsfc.nasa.gov/data/
NOAA SWPC Solar Event reports with README description of their format
ftp://ftp.swpc.noaa.gov/pub/indices/events/
Preparation for Eclipse 170821
http://herrero-victor.blogspot.com/2016/10/preparation-for-eclipse-170821.html
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Sun Earth Jupiter 2014 September

Many thanks to: STEREO and WIND Teams, Taxpayers of France, French Air Force, Nancay Decametric Array Team at the Nancay Radio Astronomy Station of Paris Observatory, Prof. Dr. Kazumasa Imai Kochi National College of Technology Kochi Japan, Trinity College Dublin Ireland Astrophysics Group, United States NOAA SWPC, NASA SDO HMI Magnetograph Team, Lockheed Martin Solar Laboratory

Periodic bursts of Jovian non-Io decametric radio emission strongly correlated with solar wind ram pressure

Periodic bursts of Jovian non-Io decametric radio emission strongly correlated with solar wind ram pressure

Panchenko, M.; Rucker, H. O.; Farrell, W. M. [ AA(Space Research Institute AAS, Graz, Austria), AB(Space Research Institute AAS, Graz, Austria), AC(NASA Goddard Space Flight Center, Greenbelt, MD, USA)] 2013

http://adsabs.harvard.edu/abs/2013P%26SS...77....3P

With many thanks to Tom Ashcraft, who brought it to my attention, I provide the link to this very interesting paper (free 2 MB pdf):

http://www.sciencedirect.com/science/article/pii/S0032063312002528/pdf?md5=d8d302c46ea00bae36dbecb5bdcc6359&pid=1-s2.0-S0032063312002528-main.pdf

 Abstract: "During the years 2000-2011 the radio instruments onboard Cassini, Wind and STEREO spacecraft have recorded a large amount of the Jovian decametric radio emission (DAM). In this paper we report on the analysis of the new type of Jovian periodic radio bursts recently revealed in the decametric frequency range. These bursts, which are non-Io component of DAM, are characterized by a strong periodic reoccurrence over several Jovian days with a period ≈1.5% longer than the rotation rate of the planet's magnetosphere (System III). The bursts are typically observed between 4 and 12 MHz and their occurrence probability has been found to be significantly higher in the sector of Jovian Central Meridian Longitude between 300° and 60° (via 360°). The stereoscopic multispacecraft observations have shown that the radio sources of the periodic bursts radiate in a non-axisymmetric hollow cone-like pattern and sub-corotate with Jupiter remaining active during several planet's rotations. The occurrence of the periodic non-Io DAM bursts is strongly correlated with pulses of the solar wind ram pressure at Jupiter. Moreover the periodic bursts exhibit a tendency to occur in groups every ˜25 days. The polarization measurements have shown that the periodic bursts are right hand polarized radio emission associated with the Northern magnetic hemisphere of Jupiter. We suggest that periodic non-Io DAM bursts may be connected with the interchange instability in Io plasma torus triggered by the solar wind."

Sun Earth Jupiter 2014 August

Many thanks to: STEREO and WIND Teams, Taxpayers of France, Nancay Decametric Array Team at Nancay Radio Astronomy Station of Paris Observatory, Prof. Dr. Kazumasa Imai Kochi National College of Technology Kochi Japan, Trinity College Dublin Ireland Astrophysics Group, United States NOAA SWPC, NASA SDO HMI Magnetograph Team, Lockheed Martin Solar Laboratory