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Found 4 entries in the Bibliography.
Showing entries from 1 through 4
2021 |
Solar probe based autonomous solar tracker system-A review The energy source which is becoming very popular nowadays is a sustainable energy source, because of the high cost and extinction of conventional fuels. One of the examples of renewable sources is solar energy. Solar energy is profusely in nature and inexhaustible energy resources around the world. The main challenge in the solar field is the less amount of solar energy captured by photovoltaic (PV) systems. To increase the efficiency of the solar power generation system we n ...
Kumar, Sarvesh; Pal, Ankur; Singh, Pallavi; Mittal, Sudhanshu; Kumar, Yatendra; Published by: 2021 International Conference on Advance Computing and Innovative Technologies in Engineering, ICACITE 2021 Published on: Photovoltaic cells; Solar energy; Solar power plants; Parker Engineering |
2020 |
Tearing Modes in Partially Ionized Astrophysical Plasma Pucci, Fulvia; Singh, Alkendra; Tenerani, Anna; Velli, Marco; Published by: \apjl Published on: 11/2020 YEAR: 2020   DOI: 10.3847/2041-8213/abc0e7 Parker Data Used; Solar magnetic reconnection; Plasma astrophysics; Space plasmas; Collision processes; 1504; 1261; 1544; 2065; Astrophysics - Solar and Stellar Astrophysics; Physics - Plasma Physics |
2019 |
Singh, K.~A.~P.; Pucci, Fulvia; Tenerani, Anna; Shibata, Kazunari; Hillier, Andrew; Velli, Marco; Published by: \apj Published on: 08/2019 YEAR: 2019   DOI: 10.3847/1538-4357/ab2b99 Parker Data Used; magnetic reconnection; magnetohydrodynamics: MHD; plasmas; Physics - Plasma Physics; Astrophysics - Solar and Stellar Astrophysics; Physics - Space Physics |
2018 |
Magnetic Helicity Reversal in the Corona at Small Plasma Beta Solar and stellar dynamos shed small-scale and large-scale magnetic helicity of opposite signs. However, solar wind observations and simulations have shown that some distance above the dynamo both the small-scale and large-scale magnetic helicities have reversed signs. With realistic simulations of the solar corona above an active region now being available, we have access to the magnetic field and current density along coronal loops. We show that a sign reversal in the horizontal averages of the magnetic helicity occurs ... Bourdin, Philippe; Singh, Nishant; Brandenburg, Axel; Published by: The Astrophysical Journal Published on: 12/2018 YEAR: 2018   DOI: 10.3847/1538-4357/aae97a Astrophysics - Solar and Stellar Astrophysics; dynamo; magnetohydrodynamics: MHD; methods: numerical; parker solar probe; Physics - Plasma Physics; Solar Probe Plus; Solar wind; Sun: corona; Sun: magnetic fields |
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