Solar Flares and the Aether Dynamic
DOI:
https://doi.org/10.55672/hij2024pp58-71Keywords:
Alfvénic Dynamics, Force-Free Model, Energy Dissipation, Aether DynamicsAbstract
This study investigates the dynamics of Solar flares using the "closed fluid dynamic principle" proposed by Muhammad Aslam Musakhail, which reinforces the pre-Einsteinian aether theory. By defining the "aether force" as the difference between relativistic total mass and rest mass, the principle provides a novel perspective on the relativistic transitions in Solar flare phenomena. The analysis builds on Parker's force-free model and Melrose’s resistive slab theory, extending them to describe the dual-phase dynamics of Solar flares: the Alfvénic phase, where massive fermions (v<c) propagate as Alfvén waves, and the heat-dissipation phase, where fermions transition to massless states (v=c), driven by current sources. Key results reveal that energy dissipation scales with resistivity, and the temporal evolution of Poynting flux and magnetic fields highlights distinct transitions between the phases. Numerical simulations demonstrate the exponential decay of axial magnetic fields and the helical organization of flux tubes. These findings validate theoretical predictions and provide insights into particle acceleration, magnetic reconnection, and energy transfer mechanisms during Solar flares. This work not only advances the understanding of Solar flare energetics but also establishes a mathematical framework that can be extended to other astrophysical phenomena, such as cosmic ray acceleration and stellar flares. Future studies should focus on numerical validation and observational testing to refine the dual-phase model and its broader applicability.
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References
D. Melrose, "Energy propagation into a flare kernel during a solar fire," vol. 387, pp. 403-413, 1992.
E. Parker, "Anomalous resistivity and the evolution of magnetic field topology," vol. 414, pp. 389-398, 1993.
D. J. S. S. R. Melrose, "The emission mechanisms for solar radio bursts," vol. 26, pp. 3-38, 1980.
G. Botha, T. Arber, V. Nakariakov, F. J. A. Keenan, and Astrophysics, "A developed stage of Alfvén wave phase mixing," vol. 363, no. 3, pp. 1186-1194, 2000.
E. N. J. A. J. Parker, vol. 128, p. 664, "Dynamics of the interplanetary gas and magnetic fields," vol. 128, p. 664, 1958.
G. Peterson and C. Chang, "Two-phase heat dissipation utilizing porous-channels of high-conductivity material," 1998.
L. D. Landau, The classical theory of fields. Elsevier, 2013.
A. J. S. P. A. W. B. Einstein, "The field equations of gravitation," vol. 1915, pp. 844-847, 1915.
A. J. S. d. K. P. A. d. W. Einstein, "Die feldgleichungen der gravitation," pp. 844-847, 1915.
J. R. Farmer, Grand unification of the four fundamental forces of physics: Amazon, 2021, p. 392. [Online]. Available.
J. R. Farmer, A saucerful of science: Amazon, 2024, p. 1072. [Online]. Available.
J. R. Farmer, Quantum theory of electrodynamics: Amazon, 2022, p. 680. [Online]. Available.
M. A. Musakhail and J. R. J. H. I. J. Farmer, "On the Aether Dynamics, Twin Paradox, and Ultimate Relativity of Solar Flares," vol. 4, no. 3, pp. 37-57. doi: https://doi.org/10.55672/hij2024pp37-57
A. J. V. d. S. N. G. Einstein, "Concerning the aether," vol. 105, no. 2, pp. 85-93, 1924.
P. M. Atkinson and S. J. P. E. Nlend, "Aether dynamics: Classical mechanics explained," vol. 36, no. 2, pp. 129-139, 2023.
C. J. S. s. r. De Jager, "Solar flares and particle acceleration," vol. 44, no. 1, pp. 43-90, 1986.
B. V. Somov, Physical processes in solar flares. Springer Science & Business Media, 1991.
E. Tandberg-Hanssen and A. G. Emslie, The physics of solar flares. Cambridge University Press, 1988.
T. Bai, P. J. I. A. r. o. a. Sturrock, and C. astrophysics. Volume 27 . Palo Alto, Annual Reviews, Inc., , p. 421-467., "Classification of solar flares," vol. 27, pp. 421-467, 1989.
A. Hasegawa and L. J. P. R. L. Chen, "Plasma heating by Alfvén-wave phase mixing," vol. 32, no. 9, p. 454, 1974.
A. Keiling, J. Wygant, C. Cattell, F. Mozer, and C. J. S. Russell, "The global morphology of wave Poynting flux: Powering the aurora," vol. 299, no. 5605, pp. 383-386, 2003.
G. Perry, K. Ruzic, K. Sterne, A. Howarth, and A. J. R. S. Yau, "Modeling and validating a SuperDARN radar's Poynting flux profile," vol. 57, no. 3, pp. 1-17, 2022.
Y.-Z. Chu, H. Mathur, T. J. P. R. D. P. Vachaspati, Fields, Gravitation,, and Cosmology, "Aharonov-Bohm radiation of fermions," vol. 82, no. 6, p. 063515, 2010.
D. Rust and A. J. S. p. Kumar, "Helical magnetic fields in filaments," vol. 155, pp. 69-97, 1994.
R. J. P. Lysak and C. o. t. Earth, "Propagation of Alfvén waves through the ionosphere," vol. 22, no. 7-8, pp. 757-766, 1997.
A. J. J. o. A. Keiling and S.-T. Physics, "The dynamics of the Alfvénic oval," vol. 219, p. 105616, 2021.
C. E. J. G. r. l. Seyler Jr, "Nonlinear 3‐D evolution of bounded kinetic Alfvén waves due to shear flow and collisionless tearing instability," vol. 15, no. 8, pp. 756-759, 1988.
V. E. J. J. o. H. E. P. Ambruş, "Helical massive fermions under rotation," vol. 2020, no. 8, pp. 1-68, 2020.

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