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Updated: Nov 10, 2025

Structural Design and Manufacturing of a Cruiser Class Solar Vehicle
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Scaling Laws for Dynamic Solar Loops.

Stephen J Bradshaw1, A Gordon Emslie2

  • 1Department of Physics & Astronomy, Rice University, Houston, TX 77005, USA.

The Astrophysical Journal
|April 2, 2021
PubMed
Summary
This summary is machine-generated.

New scaling laws for dynamic coronal loops reveal that enthalpy flux impacts energy balance. These laws are similar to static cases but depend on flow Mach number, especially in turbulent conditions.

Keywords:
Suncorona – Suncoronal loops

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Area of Science:

  • Plasma physics
  • Solar physics
  • Astrophysics

Background:

  • Established scaling laws for static coronal loops are crucial for solar physics research.
  • Dynamic coronal loops involve enthalpy flux, which is important for energy balance.

Purpose of the Study:

  • Extend existing scaling laws to dynamic coronal loops.
  • Investigate impulsive heating and filling characterized by upward enthalpy flows.
  • Analyze the impact of enthalpy flux on energy balance in dynamic loops.

Main Methods:

  • Developed new scaling laws for dynamic coronal loops.
  • Analyzed collision-dominated thermal conduction.
  • Investigated turbulent processes limiting thermal conduction.

Main Results:

  • For collision-dominated conduction, scaling laws retain functional dependencies from static cases but vary with Mach number (M).
  • Low to moderate Mach number flows show scaling laws nearly identical to static cases.
  • Turbulent conduction introduces a limiting Mach number for enthalpy fluxes between the corona and chromosphere.

Conclusions:

  • The new scaling laws provide a framework for understanding energy transport in dynamic coronal loops.
  • Mach number is a critical parameter influencing scaling laws in dynamic scenarios.
  • Turbulence plays a significant role in limiting enthalpy flux and establishing return flow dynamics.