Development of a Magnetic Loop Antenna for the Detection of Jovian Radiowaves at 20.1 MHz
Radio waves coming from the planet Jupiter are electromagnetic phenomena generated by synchrotron emission mechanism, due to the interaction of Jovian magnetic field with charged particles produced by the satellite Io. These radio waves fall directly upon the ionosphere affecting earth’s radio communications. At the Astronomical Observatory of the University of Technology of Pereira (OAUTP) the research group in Astro-engineering Alfa Orion, developed a magnetic loop antenna designed to resonate at 20.1 MHz, which coupled with the receptor and the software from NASA’s Radio Jove project enabled the observation of radio sources A, B, C, IoA, IoB and IoC from Jupiter, allowing the construction of a database for the study of the Jovian activity in radio waves.
F. Burke and K. L. Franklin. “Observations of a variable radio source associated with the planet Jupiter”, JGR., vol. 2, no.
, pp. 213-217, 1955. Available: http://adsabs.harvard.edu/abs/1955JGR....60..213B
M. Wilkinson and J. Kennewell. “Detecting Jupiter's radio emissions”, Aug, 2013. [Online]. Available: http://www.spaceacademy.net.au/spacelab/projects/jovrad/jovrad.htm
D. Basu and J. L. Pires. “Relation between Jupiter's Decametric Radio Emission and its Great Red Spot”, Astrophysical Letters, vol. 12 pp. 99-102, 1972. Available: http://adsabs.harvard.edu/abs/1972ApL....12...99B
D. Basu and C. J. Banos. “Relation between Jupiter's decametric radio emission and its activity in the equatorial zone”, Astrophysical Letters, vol. 16, pp. 97-100, 1975. Available: http://adsabs.harvard.edu/abs/1975ApL....16...97B
K. M. Abood and R. H. Ibrahim. “Relationship between CML and Io's phase according to Jupiter's actual radio storms observations”, IJP, vol. 11, no. 20, pp. 100-109, 2013.
A. B. Bhattacharya and S. Mondal. “Probability of Reception of Jovian Bursts as Derived from Io-Phase and the Location of Central Meridian Longitude”, IJECT, vol. 4, pp. 104-106, 2013.
B. Ismail and M. K. Hisham. “Listening to Jupiter's signal using Radio Telescope Recorder”, ICCDA, vol. 1, pp. 278-282, 2010.
A. B. Bhattacharya et al., “Detection Of Jovian Radio Bursts At High Altitudes,” IJEST, vol. 4, no. 06, pp. 3029-3038, 2012.
R. S. French. “An urban radio telescope for Jovian and solar emissions at 20.1 MHz” SAO, Nov, 2009. [Online]. Available: http://rfrench.org/astro/papers/P143-HET608-RobertFrench.pdf
S. Joardar and A. B. Bhattacharya. “Design and analysis of a low-frequency radio telescope for Jovian radio emission”, Electromagnetics Research, vol. 72, pp. 127-143, 2007. Available: http://adsabs.harvard.edu/abs/2007PrER...72..127J
J. L. Lombardero. “Radiotelescopio loop” CPAN-Ingenio, pp. 1-16, 2010, https://www.i-cpan.es/concurso4/docs/radiotelescopio-loop.pdf
W. Kwon et al., “A magnetic resonant loop antenna to enhance the operating distance of 13.56 MHz RFID systems”, ISOCC IEEE, pp. 013-014, 2013.
F. El Hatmi et al. “Magnetic loop antenna for wireless capsule endoscopy inside the human body operating at 315 MHz: Near field behavior,” MMS IEEE, pp. 81-87, 2011.
H. Martinez and M. R Ghezzi. “La antenna cuadro o Magnetic loop,” SOLVEGJ Comunicaciones, pp. 1-13, 2014. [Online]. Available: http://lu6etj.host-argentina.com.ar/lu6etj/tecnicos/loop/antena_de_cuadro.htm
J. D. Kraus, Antennas. New Delhi, USA: McGraw Hills, Press 1997. Ch. 6.
N. K. Nikolova, Hamilton, Loop Antennas. Canada, 2014, [Online]. Available: http://www.antentop.org/004/files/tr004.pdf
S. Yates, “Small Transmitting Loop Antennas: Magnetic Loop Antennas,” Texas, USA, 2013. [Online]. Available: http://www.aa5tb.com/loop.html
A. Voors, “4Nec2 based antenna modeler and optimizer”, 2005. [Online]. Available: http://www.qsl.net/4nec2/
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