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The solar dynamo is essentially a cyclic process in which the toroidal component of the magnetic field is converted into the poloidal one and vice versa. This cyclic loop is disturbed by some nonlinear and stochastic processes mainly operating in the
Externí odkaz:
http://arxiv.org/abs/2403.06176
Publikováno v:
In Advances in Space Research 1 February 2024 73(3):2119-2132
Publikováno v:
Cluster Computing; Sep2024, Vol. 27 Issue 6, p7889-7914, 26p
Publikováno v:
In Advances in Space Research 1 January 2022 69(1):798-813
Autor:
Prasad, Amrita1 (AUTHOR) prasad.amrita1@gmail.com, Roy, Soumya2 (AUTHOR), Sarkar, Arindam3 (AUTHOR), Panja, Subhash Chandra1 (AUTHOR), Patra, Sankar Narayan4 (AUTHOR)
Publikováno v:
Solar Physics. Mar2023, Vol. 298 Issue 3, p1-20. 20p.
Autor:
Singh, Ragini1 (AUTHOR), Prasad, Amrita2 (AUTHOR), Kumar, Binayak1 (AUTHOR), Kumari, Soni1 (AUTHOR), Sahu, Ram Krishna1 (AUTHOR), Hedau, Suresh T.1 (AUTHOR) suresh.hedau@gov.in
Publikováno v:
ChemistrySelect. 9/27/2022, Vol. 7 Issue 36, p1-18. 18p.
Autor:
Tiwari, Mahavir Prasad, Prasad, Amrita
Publikováno v:
In Analytica Chimica Acta 1 January 2015 853:1-18
Autor:
Prasad, Amrita1 (AUTHOR) prasad.amrita1@gmail.com, Roy, Soumya2 (AUTHOR), Ghosh, Koushik3 (AUTHOR), Panja, Subhash Chandra1 (AUTHOR), Patra, Sankar Narayan4 (AUTHOR) sankar.journal@gmail.com
Publikováno v:
Solar System Research. Mar2021, Vol. 55 Issue 2, p169-182. 14p.
Publikováno v:
In Colloids and Surfaces B: Biointerfaces 1 January 2014 113:69-76
Akademický článek
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