• → European Space Agency

      • Space for Europe
      • Space News
      • Space in Images
      • Space in Videos
    • About Us

      • Welcome to ESA
      • DG's News and Views
      • For Member State Delegations
      • Business with ESA
      • ESA Exhibitions
      • ESA Publications
      • Careers at ESA
    • Our Activities

      • Space News
      • Observing the Earth
      • Human Spaceflight
      • Launchers
      • Navigation
      • Space Science
      • Space Engineering
      • Operations
      • Technology
      • Telecommunications & Integrated Applications
    • For Public

    • For Media

      • Media
      • ESA TV
      • Videos for professionals
      • Photos
    • For Educators

    • For Kids

    • ESA

    • Space in Images

    ESA > Space in Images > 2010 > 04 > SOHO uses an internal occulting disk

    Free Search (10912 images)

    • Recently Added
    • Advanced Search

    SOHO uses an internal occulting disk

    (3.23 MB)
    Views: 13
    Rating: 0.00/5 (0 votes cast)

    Rate this Image

    • Currently 0 out of 5 Stars.
    • 1
    • 2
    • 3
    • 4
    • 5

    Thank you for rating!

    You have already rated this page, you can only rate it once!

    Your rating has been changed, thanks for rating!

    Share this Image

    Post to Facebook Post to MySpace Post to Delicious Post to Digg Post to Twitter

    Details

    Open/Close
    • Title SOHO uses an internal occulting disk
    • Released 05/02/2007 2:05 pm
    • Copyright ESA/NASA
    • Description

      SOHO uses an internal sun-shade known as an occulter to view the corona, but diffraction of stray light limits the area that can be observed. The bright circle within the dark disk shows the actual size and position of the Sun. SOHO's occulter covers twice the diameter of the Sun. The external coronagraph planned for Proba-3 will cover only 1.05 solar radii, or even less, so a previously hidden section of the corona will be visible on a sustained basis.

      The Sun unleashed a large (X-3 class) solar flare December 13, 2006 along with a coronal mass ejection (CME) that appears to be headed towards Earth. The source of these eruptions was the very active sunspot region 930. A shower of high-energy particles appeared as specks and white streaks on the imagers aboard SOHO, the primary watchdog for solar storms. The video clip from LASCO C2 coronagraph shows a CME emerging from behind the occulting disk and then almost immediately the imager is being struck by the particles (that travel at half the speed of light).


    TAGS

    Open/Close
    • Click on the tags to find the matching images.
    • Activity Space Science
    • Mission SOHO , Space Situational Awareness (SSA)
    • Keywords , Sunspots

    TAGS

    Open/Close

    Details

    Open/Close

    RELATED IMAGES

    • Large solar flare, 13 December 2006
      Released: 05/02/2007
      Rating
    • Solar flare 31 August 2012 seen by SOHO
      Solar flare seen by SOHO
      Released: 03/01/2013
      Rating

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Facebook
    • Livestream
    • Subscribe
    • App Store
    • LATEST ARTICLES
    • · Rare merger reveals secrets of g…
    • · Watching for hazards: ESA opens …
    • · ESA astronaut Timothy Peake set …
    • · Space drives e-mobility
    • · Proba-V opens its eyes
    • FAQ

    • Jobs at ESA

    • Site Map

    • Contacts

    • Terms and conditions