The Time-Scalar Origin of Solar Coronal Heating and Wind Acceleration

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Main Author: Farrell, Jordan Gabriel
Format: Recurso digital
Language:English
Published: Zenodo 2025
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_version_ 1866902005228765184
author Farrell, Jordan Gabriel
author_facet Farrell, Jordan Gabriel
contents <p>The solar coronal heating paradox involves the corona reaching temperatures of 1–3 MK while the photosphere remains at ≈5800 K. Classical magnetohydrodynamic (MHD) mechanisms, such as Alfv´en wave dissipation and nanoflares, fail to quantitatively account for this inversion. We introduce Time-Scalar Field Theory (TSFT), where a scalar-time gradient ∇ΘΦ provides an additional energy transfer term neglected in MHD, predicting exponential amplification in regions of high temporal curvature. This mechanism aligns with empirical data from missions like Parker Solar Probe, SDO/AIA, and Hinode/EIS, yielding a Pearson correlation of -0.974 (p = 0.001) between predicted and observed electron temperatures. We extend the model to explain solar wind acceleration, showing that the same scalar-time curvature produces continued outward momentum beyond the coronal base.</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_18064351
institution Zenodo
language eng
publishDate 2025
publisher Zenodo
record_format zenodo
spellingShingle The Time-Scalar Origin of Solar Coronal Heating and Wind Acceleration
Farrell, Jordan Gabriel
Theoretical physics
Time-Scalar Field Theory
Fundamental Physics
Foundations of Physics
Scalar Field Theory
<p>The solar coronal heating paradox involves the corona reaching temperatures of 1–3 MK while the photosphere remains at ≈5800 K. Classical magnetohydrodynamic (MHD) mechanisms, such as Alfv´en wave dissipation and nanoflares, fail to quantitatively account for this inversion. We introduce Time-Scalar Field Theory (TSFT), where a scalar-time gradient ∇ΘΦ provides an additional energy transfer term neglected in MHD, predicting exponential amplification in regions of high temporal curvature. This mechanism aligns with empirical data from missions like Parker Solar Probe, SDO/AIA, and Hinode/EIS, yielding a Pearson correlation of -0.974 (p = 0.001) between predicted and observed electron temperatures. We extend the model to explain solar wind acceleration, showing that the same scalar-time curvature produces continued outward momentum beyond the coronal base.</p>
title The Time-Scalar Origin of Solar Coronal Heating and Wind Acceleration
topic Theoretical physics
Time-Scalar Field Theory
Fundamental Physics
Foundations of Physics
Scalar Field Theory
url https://doi.org/10.5281/zenodo.18064351