Stock Photo: Coronal holes appear as dark areas of the corona when viewed in ultraviolet light and in X-rays. Coronal holes are the source of strong solar wind gusts that carry solar particles out to our magnetosphere and beyond. These images are over the span of a week, and are Extreme ultraviolet Imaging Telescope (EIT) of the Solar and Heliospheric Observatory (SOHO), at a wavelength of 284 angstroms.

Coronal holes appear as dark areas of the corona when viewed in ultraviolet light and in X-rays. Coronal holes are the source of strong solar wind gusts that carry solar particles out to our magnetosphere and beyond. These images are over the span of a week, and are Extreme ultraviolet Imaging Telescope (EIT) of the Solar and Heliospheric Observatory (SOHO), at a wavelength of 284 angstroms. : Stock Photo

4389-1635 | Rights Managed
Credit: NASA / NASA
Category: Science
scf4571-034

Release Details

Model Release: No
Property Release: No

Please Contact

SuperStock Sales and Research
Email: yourfriends@superstock.com
Phone: 1-800-828-4545
Fax: 1-904-565-1620

Max
  • 23.62" x 9.04"
  • 300 dpi
  • 54.96MB