TY - GEN
T1 - Correlation between the Jupiter-Io Observations and the Solar Radio Bursts using the Sharjah Decametric Radio Telescope (SDRT)
AU - Yousef, Areej
AU - Rihan, Mohammad
AU - Shuhail, Salem
AU - Hindawi, Noor Al
AU - Madara, Sahith Reddy
AU - Fernini, Ilias
AU - Al-Naimiy, Hamid M.K.
N1 - Publisher Copyright:
Copyright ©2021 by the International Astronautical Federation (IAF). All rights reserved.
PY - 2021
Y1 - 2021
N2 - This paper will look into the factors that affect the correlation between the Jupiter-Io observed radio events and the Sun radio bursts using the Sharjah Decametric Radio Telescope (SDRT) located at the Sharjah Academy for Astronomy, Space Sciences, and Technology in the United Arab Emirates. The SDRT has been operational since 2019 and is sponsored by the UAE Space Agency. We analyze the number of Jupiter and Sun events to the Sun cycle's predicted events from 2019 to 2020 related to the solar cycles 25 and 25. One factor that affected our Jovian-Io observations is the apparent angle between the Sun and Jupiter. We have noticed that these events are at a maximum during opposition and minimum during the conjunction. Some Jovian events were predicted by the Radio-Jupiter Pro III software but were not detected by the SDRT. We show a modest correlation between the observed solar flares and the trapped particle flux at Io's orbit responsible for Jupiter's radio L- and S-bursts. These observations are essential to understand the Jupiter-Io exchange of particles due to its moon Io volcanic nature and Jupiter's intense magnetic field enhanced by the solar radio bursts observed by the SDRT.
AB - This paper will look into the factors that affect the correlation between the Jupiter-Io observed radio events and the Sun radio bursts using the Sharjah Decametric Radio Telescope (SDRT) located at the Sharjah Academy for Astronomy, Space Sciences, and Technology in the United Arab Emirates. The SDRT has been operational since 2019 and is sponsored by the UAE Space Agency. We analyze the number of Jupiter and Sun events to the Sun cycle's predicted events from 2019 to 2020 related to the solar cycles 25 and 25. One factor that affected our Jovian-Io observations is the apparent angle between the Sun and Jupiter. We have noticed that these events are at a maximum during opposition and minimum during the conjunction. Some Jovian events were predicted by the Radio-Jupiter Pro III software but were not detected by the SDRT. We show a modest correlation between the observed solar flares and the trapped particle flux at Io's orbit responsible for Jupiter's radio L- and S-bursts. These observations are essential to understand the Jupiter-Io exchange of particles due to its moon Io volcanic nature and Jupiter's intense magnetic field enhanced by the solar radio bursts observed by the SDRT.
KW - Magnetic Field
KW - Opposition
KW - Sharjah Decametric Radio Telescope
KW - Solar Cycle
KW - Solar Radio Bursts
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M3 - Conference contribution
AN - SCOPUS:85127503347
T3 - Proceedings of the International Astronautical Congress, IAC
BT - IAF Symposium on Ongoing and Near Future Space Astronomy and Solar-System Science Missions 2021 - Held at the 72nd International Astronautical Congress, IAC 2021
PB - International Astronautical Federation, IAF
T2 - IAF Symposium on Ongoing and Near Future Space Astronomy and Solar-System Science Missions 2021 at the 72nd International Astronautical Congress, IAC 2021
Y2 - 25 October 2021 through 29 October 2021
ER -