2019
DOI: 10.48550/arxiv.1908.06042
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Thermomagnetic Ettingshausen-Nernst effect in tachocline, magnetic reconnection phenomenon in lower layers, axion mechanism of solar luminosity variations, coronal heating problem solution and mechanism of ADM variations around BH

V. D. Rusov,
M. V. Eingorn,
I. V. Sharph
et al.

Abstract: It is shown that the holographic principle of quantum gravity (in the hologram of the Universe, and therefore in our Galaxy, and of course on the Sun!), in which the conflict between the theory of gravitation and quantum mechanics disappears, gives rise to the Babcock-Leighton holographic mechanism. Unlike the solar dynamo models, it generates a strong toroidal magnetic field by means of the thermomagnetic Ettingshausen-Nernst (EN) effect in the tachocline. Hence, it can be shown that with the help of the ther… Show more

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Cited by 2 publications
(26 citation statements)
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References 746 publications
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“…An interesting problem arises here related to the heating of the practically empty magnetic tube (see Figs. 6a and 11 in [8]) and heating of the solar corona, which has long been unresolved (see [29,30]). There are many assumptions about the unusually high temperature in the corona (see e.g.…”
Section: Corona Heating Problemmentioning
confidence: 99%
See 2 more Smart Citations
“…An interesting problem arises here related to the heating of the practically empty magnetic tube (see Figs. 6a and 11 in [8]) and heating of the solar corona, which has long been unresolved (see [29,30]). There are many assumptions about the unusually high temperature in the corona (see e.g.…”
Section: Corona Heating Problemmentioning
confidence: 99%
“…From now on we are interested in the energy-independent case (7) or (8) which plays the key role in determination of the parameters for the axion mechanism of Sun luminosity variations (the axion coupling constant to photons g aγ , the transverse magnetic field B of length L and the axion mass m a ).…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…For example, at strong magnetic fields of flux tubes, at B B eq , the diamagnetic effect becomes almost neg- The blue line (see also Fig. 8 in [21,155]) denotes admissible values for the standard solar model with diffusion of helium [97], with the initial value of the theoretical estimate of the magnetic field Bz ≈ 4 • 10 7 G (see Eq. ( 2)).…”
Section: B Secondary Reconnection Of Magnetic Tubes In Lower Layers A...mentioning
confidence: 99%
“…(a)Change in the magnetic field strength Bz along the rising Ω-loop as a function of the Sun depth R/RSun in the convective zone. The blue line (see also Fig.8in[21,155]) denotes admissible values for the standard solar model with diffusion of helium[97], with the initial value of the theoretical estimate of the magnetic field Bz ≈ 4 • 10 7 G (see Eq. (2)).…”
mentioning
confidence: 99%