Related Experiment Video
Updated: Jul 9, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
Chromospheric alfvenic waves strong enough to power the solar wind
B De Pontieu1, S W McIntosh, M Carlsson
1Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Organization ADBS, Building 252, Palo Alto, CA 94304, USA. bdp@lmsal.com
Strong Alfvén waves were detected in the Sun's chromosphere, providing a potential explanation for solar wind acceleration and coronal heating. These observations bridge a critical gap in understanding solar atmospheric dynamics.
Area of Science:
- Solar Physics
- Plasma Physics
- Astrophysics
Background:
- Alfvén waves are theorized to heat the Sun's corona and accelerate the solar wind.
- Direct observation of sufficiently strong Alfvén waves in the solar atmosphere has been lacking.
Purpose of the Study:
- To investigate the presence and characteristics of Alfvén waves in the solar atmosphere.
- To determine if observed Alfvén waves possess sufficient energy for coronal heating and solar wind acceleration.
Main Methods:
- Utilized high temporal and spatial resolution images from the Solar Optical Telescope on the Hinode satellite.
- Analyzed wave properties within the chromosphere, the layer between the solar surface and corona.
Main Results:
- Detected Alfvén waves with significant amplitudes (10-25 km/s) and periods (100-500 s) permeating the chromosphere.
- Estimated the energy flux carried by these waves.
Conclusions:
- The observed Alfvén waves are energetic enough to potentially accelerate the solar wind.
- These waves may also contribute to heating the quiet solar corona.
Related Concept Videos
Momentum And Radiation Pressure
Energy Carried By Electromagnetic Waves
Nuclear Fusion
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
Radiation Pressure: Problem Solving
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...
Faraday Disk Dynamo
Electromagnetic Waves in Matter
Consider the electromagnetic wave passing through a dielectric medium. In such a case, Maxwell's equations get modified. In Ampere's law, ε0 , the dielectric permittivity of free space is replaced with ε, the permittivity of dielectric. Also, the vacuum permeability μ0 is replaced by the permeability of the medium, μ.
Furthermore, the...

