TY - JOUR
T1 - Sharjah-Sat-3 Mission Design Analysis with STK Software
T2 - 74th International Astronautical Congress, IAC 2023
AU - Alhammadi, Amel
AU - Alansaari, Maryam
AU - Alketbi, Fatima
AU - Faroukh, Yousuf
AU - Sulaiman, Abdulrahman
AU - Altunaiji, Ahmed
AU - AlKaabi, Tarifa
AU - Fernini, Ilias
AU - Al-Naimiy, Hamid M.K.
N1 - Publisher Copyright:
Copyright © 2023 by the International Astronautical Federation (IAF). All rights reserved.
PY - 2023
Y1 - 2023
N2 - The Sharjah Academy for Astronomy, Space Sciences, and Technology (SAASST) is currently developing a new 6U low-cost CubeSat, Sharjah-Sat-3, a space weather satellite to monitor the daily behavior of the ionosphere layer due to the activity of the Sun. This is part of the "Space Weather" program the United Arab Emirates is pursuing to preserve its space assets. Sharjah-Sat-3's main payload is a solar particle detector (SPD) to measure the charged particles' density of electrons, protons, and ions in the energy range of 0.1-100 MeV. This range is the expected energies of these particles at the LEO level. When designing such a complex space mission, many factors must be considered before implementing, selecting, and procuring the components. This consideration could be performed by simulating and modeling the scenario of the system. This paper will conduct a simulation analysis for the proposed mission design using system tool kit (STK) software in three different orbits in three different approaches. The first one is estimating the optimal orbit for the ground-space telecommunication side, which shows how often our Satellite will pass over the ground station. The second is the lifetime analysis, which indicates how long the Satellite will stay in orbit. The last approach is determining the generated power by the selected solar panel configuration and evaluating the results according to each subsystem's requirements. In addition, this paper will highlight the SPD payload and its efficiency in measuring the different particle densities in our ionosphere. A solar eruption is an intense source of extreme ultraviolet radiation. This changes the ionospheric ionization and produces electrons, protons, and ions that interact chemically with the atmospheric element before reaching the ground level. The most energetic solar activity happens in the polar ionosphere region. This is why we plan to include the polar orbit region in the analysis. Our determinations will aid decision-making through practical trade-off analysis and assist in setting policies towards adverse space weather effects while advising the aviation authority on space weather hazards.
AB - The Sharjah Academy for Astronomy, Space Sciences, and Technology (SAASST) is currently developing a new 6U low-cost CubeSat, Sharjah-Sat-3, a space weather satellite to monitor the daily behavior of the ionosphere layer due to the activity of the Sun. This is part of the "Space Weather" program the United Arab Emirates is pursuing to preserve its space assets. Sharjah-Sat-3's main payload is a solar particle detector (SPD) to measure the charged particles' density of electrons, protons, and ions in the energy range of 0.1-100 MeV. This range is the expected energies of these particles at the LEO level. When designing such a complex space mission, many factors must be considered before implementing, selecting, and procuring the components. This consideration could be performed by simulating and modeling the scenario of the system. This paper will conduct a simulation analysis for the proposed mission design using system tool kit (STK) software in three different orbits in three different approaches. The first one is estimating the optimal orbit for the ground-space telecommunication side, which shows how often our Satellite will pass over the ground station. The second is the lifetime analysis, which indicates how long the Satellite will stay in orbit. The last approach is determining the generated power by the selected solar panel configuration and evaluating the results according to each subsystem's requirements. In addition, this paper will highlight the SPD payload and its efficiency in measuring the different particle densities in our ionosphere. A solar eruption is an intense source of extreme ultraviolet radiation. This changes the ionospheric ionization and produces electrons, protons, and ions that interact chemically with the atmospheric element before reaching the ground level. The most energetic solar activity happens in the polar ionosphere region. This is why we plan to include the polar orbit region in the analysis. Our determinations will aid decision-making through practical trade-off analysis and assist in setting policies towards adverse space weather effects while advising the aviation authority on space weather hazards.
KW - Access Time
KW - CubeSat
KW - Lifetime
KW - Sharjah-Sat-3
KW - Solar Flare
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M3 - Conference article
AN - SCOPUS:85188004384
SN - 0074-1795
VL - 2023-October
JO - Proceedings of the International Astronautical Congress, IAC
JF - Proceedings of the International Astronautical Congress, IAC
Y2 - 2 October 2023 through 6 October 2023
ER -