Welcome to Starlight Cascade Observatory Radio Jove Project !
Near Yarker, Ontario, Canada.
(44.22.39 N 76.45.47 W 155M Elevation)
Page Created: 2010 June 29
Page Last Updated: 2024 March 01
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Current Status (last changed 2017 Nov 08): Dual dipole Antenna Mast height = 15', Phase cable 90 deg south dipole, beam center elevation 49 deg, Jupiter elevation from 45 deg Latitude: 35 degrees. So the beam is still aimed a little high.. 49-35=14 degrees high.
Changing from a 90 deg to a 135 degree phasing cable would lower the beam center from 49 degrees to 42 degrees.
TODO build a 135 degree phasing cable length 12.12' and replace 90 degree phasing cable (length=8.08')
In 2023 Jupiter elevation angle will be 45 degrees, so the antenna and Jupiter will be ideally configured.
Radio JOVE students and amateur scientists observe and analyze natural radio emissions of Jupiter, the Sun, and our galaxy.
The Radio JOVE project is a hands-on inquiry-based educational project that allows students, teachers and the general public to learn about radio astronomy by building their own radio telescope from an inexpensive kit and/or using remote radio telescopes through the internet. Participants also collaborate with each other through interactions and sharing of data on the network. The Radio JOVE project began in 1998. Since then, more than 1100 teams of students and interested individuals have purchased our non-profit radio telescope kits and are learning radio astronomy by building and operating a radio telescope. This self-supporting program continues to thrive and inspire new groups of students as well as individuals. |
2022 March 14
Dear Radio Enthusiast,
The Radio JOVE Project is pleased to announce Radio JOVE 2.0, an exciting NASA Partner citizen science project where participants purchase, assemble, and operate a 16-24 MHz radio spectrograph to observe solar, Jupiter, Galactic, and Earth-based radio emissions. Participants have a path to become a citizen scientist capable of contributing scientific-quality data to our data archive. We will continue to support both hardware and software for those participants with RJ1.1 receivers (and calibrators) and we encourage those observers to participate in our citizen science projects. Read the full announcement in our Special Bulletin: https://radiojove.gsfc.nasa.gov/newsletters/ As part of our new direction into citizen science, Radio JOVE has also upgraded our listserv. Register with our Groups.io group (https://groups.io/g/radio-jove) and receive discussions about the Radio JOVE project. This listserv is an invaluable source of information relating to all things Radio JOVE. The old listserv will be turned off by April 15, 2022, so we strongly encourage participants to move to our Groups.io list to continue communicating with us and receiving RJ information. Visit our Getting Started webpage for more about how to participate in Radio JOVE. We are excited to start this new science adventure with you. Best regards, The Radio JOVE Team |
https://services.swpc.noaa.gov/images/swx-overview-small.gif
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https://www.radiojove.net/SUG/Software/SDRuno_Installer_1.33.exe
Over 20 years of images, sounds and data files of radio observations of Jupiter, the Sun and the Galaxy is currently available for searching on the Radio JOVE Archive.
The dual dipole antennas set to 15' above ground aligned to geographic east/west. |
We plan to build the receiver assembly in the next week, find some RG6 coax to run from the combiner to the receiver and then finding some spare computer to take the audio output from the receiver and run it through a data recorder such as skypipe.
We need approx 70' of coax to run from the antenna to the observatory building where the computer will be. Using RG6 coax (we could not find any RG59) we determined that the nearest 0.5 wavelength that is at least that long is 2.5 wavelengths of 38.18' (11.64m) or 95.45' (29.1m) in total. Luckily our local Rona hardware store sells a 30m roll of RG6 for only $40 or so.
Jupiters declination in mid 2010 is approx 0 degrees and is increasing. It's elevation based on our latitude of approx 45 degrees will be approx 45 degrees and increasing.
The antenna height above ground for 40-55 degrees is 15', so we assembled the mast for that height.
JEA=JupiterElevationAngle; AH=AntennaHeight 2010 Jul1 JEA=45deg AH=15' manuals/2011 Jan1 JEA=43deg AH=15' 2011 Jul1 JEA=56deg AH=10' 2012 Jan1 JEA=55deg AH=15' 2012 Jul1 JEA=65deg AH=10' 2013 Jan1 JEA=65deg AH=10'