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An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container.
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The evolution of the solar wind.

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  • 1School of Physics, Trinity College Dublin, The University of Dublin, Dublin-2, Ireland.

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Summary
This summary is machine-generated.

This review explores the solar wind's evolution over billions of years, linking stellar properties like rotation and magnetism to mass-loss rates. Understanding this evolution impacts our view of planetary habitability and exoplanetary systems.

Keywords:
Solar windStars: activity, magnetism, rotationStellar winds and outflowsStellar winds: observations and models

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Area of Science:

  • * Astrophysics
  • * Heliophysics
  • * Planetary Science

Background:

  • * The solar wind, a stream of charged particles released from the upper atmosphere of the Sun, has evolved significantly over billions of years.
  • * Its properties are intrinsically linked to the Sun's rotation, magnetic field, and overall activity.
  • * Direct measurements of the ancient solar wind are impossible, necessitating indirect methods.

Purpose of the Study:

  • * To review the long-term evolution of the solar wind.
  • * To place the Sun and its wind within a broader stellar context using stellar data.
  • * To discuss the implications of solar wind evolution on Earth and other planets.

Main Methods:

  • * Analysis of stellar data from solar-like stars to infer past solar wind properties.
  • * Overview of detection methods for stellar winds.
  • * Derivation of an evolutionary sequence for solar wind mass-loss rates.
  • * Linking observational stellar properties with theoretical stellar wind models.

Main Results:

  • * An observed evolutionary sequence of solar wind mass-loss rates has been derived from stellar data.
  • * Key properties like stellar rotation, magnetism, and activity are correlated with solar wind characteristics.
  • * The evolution of the solar wind has had significant implications for the development of Earth and other planets.

Conclusions:

  • * The study of exoplanetary systems offers new perspectives for understanding solar wind evolution.
  • * Understanding the Sun's past wind is crucial for comprehending planetary evolution and habitability.
  • * Continued research integrating stellar and solar wind data is vital.