Loading presentation...

Present Remotely

Send the link below via email or IM

Copy

Present to your audience

Start remote presentation

  • Invited audience members will follow you as you navigate and present
  • People invited to a presentation do not need a Prezi account
  • This link expires 10 minutes after you close the presentation
  • A maximum of 30 users can follow your presentation
  • Learn more about this feature in our knowledge base article

Do you really want to delete this prezi?

Neither you, nor the coeditors you shared it with will be able to recover it again.

DeleteCancel

Make your likes visible on Facebook?

Connect your Facebook account to Prezi and let your likes appear on your timeline.
You can change this under Settings & Account at any time.

No, thanks

The Layers of the Sun's Atmosphere

This will explain the different layers of the sun's atmosphere, how hot they are, and the distinct features of each layer.
by

james schmidt

on 21 February 2011

Comments (0)

Please log in to add your comment.

Report abuse

Transcript of The Layers of the Sun's Atmosphere

The Layers of the Sun's Atmosphere The Photosphere The Photoshpere is 5800K (9980.6 ºF). The Chromoshpere The Chromosphere is a thin layer that is 10,000K (17540.6 ºF). The Layers of the Sun's Atmosphere are the Photosphere, the Chromosphere and the Corona. The Corona This is the outermost layer of the sun, it is 1,000,000 km thick, it has a temperature of about 1,000,000 K (1799540.6 ºF).
. Source: phobos.physics.uiowa.edu/~kaaret/sgu_s05/L09_sun_outer.ppt The picture was a sunspot. They are located in the Photosphere. The picture was a coronal mass ejection.
They can damage Earth's satellites that we use for our cell phones. They also cause the Aurora Lights. Source: phobos.physics.uiowa.edu/~kaaret/sgu_s05/L09_sun_outer.ppt Solar Flare These can be
up to 40,000,000 K
(71999540.6 ºF) This is the approximate size of the
Earth compared to a solar flare. These are relitavely similar to coronal mass ejections. This layer can only be seen during a solar eclipse. This layer is hotter than the photosphere (the inner layer). The reason why is unknown. This layer emits a high energy radiation that can be observed using X rays. This is the layer of the sun's
atmosphere that we can see
all the time during the day
without clouds. Each of these layers have
a different tempurature. The rotation of the sun is measured with the sunspots in the photospere. The Equator takes about 25 days for a full rotation while the poles take up to 36 days.
Full transcript