TOPOLOGICAL PHASE TRANSITION III: SOLAR SURFACE ERUPTIONS AND SUNSPOTS - Archive ouverte HAL Accéder directement au contenu
Pré-Publication, Document De Travail Année : 2018

TOPOLOGICAL PHASE TRANSITION III: SOLAR SURFACE ERUPTIONS AND SUNSPOTS

Tian Ma
  • Fonction : Auteur
  • PersonId : 1012281
Shouhong Wang
  • Fonction : Auteur
  • PersonId : 1012282

Résumé

This paper is aimed to provide a new theory for the formation of the solar surface eruptions and sunspots. The key ingredient of the study is the new anti-diffusive effect of heat, based on the recently developed statistical theory of heat by the authors [3]. The anti-diffusive effect of heat states that due to the higher rate of photon absorption and emission of the particles with higher energy levels, the photon flux will move toward to the higher temperature regions from the lower temperature regions. This anti-diffusive effect of heat leads to a modified law of heat transfer, which includes a reversed heat flux counteracting the heat diffusion. It is this anti-diffusive effect of heat and thereby the modified law of heat transfer that lead to the temperature blow-up and consequently the formation of sunspots, solar eruptions, and solar prominences. Such anti-diffusive effect of heat may be utilized to design instruments for a plasm fuel.
Fichier principal
Vignette du fichier
tpt3.pdf (460.8 Ko) Télécharger le fichier
Origine : Fichiers produits par l'(les) auteur(s)
Loading...

Dates et versions

hal-01672381 , version 1 (24-12-2017)
hal-01672381 , version 2 (14-09-2018)
hal-01672381 , version 3 (19-09-2018)

Identifiants

  • HAL Id : hal-01672381 , version 3

Citer

Tian Ma, Shouhong Wang. TOPOLOGICAL PHASE TRANSITION III: SOLAR SURFACE ERUPTIONS AND SUNSPOTS. 2018. ⟨hal-01672381v3⟩
107 Consultations
120 Téléchargements

Partager

Gmail Facebook X LinkedIn More