The DIFFERENTIAL rotation of the Sun and ITS Chromosphere

The Sun is not a solid body, its gaseous composition allows different rotation speeds on its surface, that is, different angular velocities. This is what we call "differential rotation" and it also occur in other gaseous planets such as Jupiter or Saturn. We can use an h-alpha telescope to observe this phenomena and also learn about one of the thinnest and hottest layers of the Sun: the Chromosphere.

THE DOCUMENTS: 

• The booklet
• Student's guide 
• Teacher's guide
• Formula sheet
• Calculations and results blank sheet

THE SOFTWARE:

• Calculate the differential rotation
• Heliographic coordinates

DEMO IMAGES:

• CESAR Solar Observatory

QUIZ:

Example:

• Quiz for students
• Quiz for teachers

USEFUL LINKS/WEBSITES:

• Video explaning the rotation
• What are solar flares?
• Solar Orbiter ESA