The Solar Wind.pdf

The Solar Wind.pdf The Solar Wind.pdf

igpp.ucla.edu
from igpp.ucla.edu More from this publisher
10.07.2015 Views

• Waves and turbulence?– One possibility is that the corona is heated by compressionalwaves at or just below the surface. Oscillatory motion of theSun’s surface could drive pressure waves. In theory fastmode waves could propagate up to 20R Sun . Experimentsdesigned to detect sound waves propagating into the coronahave not detected them.• Impulsive energy release?– The Sun has a magnetic field that contains magnetic energy.Magnetic energy can be converted into thermal energy. Thisis done by reconnection. The granularity of the photosphereas the top of the convection zone is caused by bubbles risingand falling. These might reconnect. X-ray bursts may beevidence of this happening.• We still don’t know how the corona is heated!

• Motion of granules and magnetic structures –Hinode observations

• Waves and turbulence?– One possibility is that the corona is heated by compressionalwaves at or just below the surface. Oscillatory motion of theSun’s surface could drive pressure waves. In theory fastmode waves could propagate up to 20R Sun . Experimentsdesigned to detect sound waves propagating into the coronahave not detected them.• Impulsive energy release?– <strong>The</strong> Sun has a magnetic field that contains magnetic energy.Magnetic energy can be converted into thermal energy. Thisis done by reconnection. <strong>The</strong> granularity of the photosphereas the top of the convection zone is caused by bubbles risingand falling. <strong>The</strong>se might reconnect. X-ray bursts may beevidence of this happening.• We still don’t know how the corona is heated!

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!