SDO First Light

These are "First Light" release movies for Solar Dynamics Observatory (SDO). For more information about SDO, visit the SDO web site @ NASA.gov.

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Press Release Materials

SDO Atmospheric Imaging Assembly (AIA)

The Atmospheric Imaging Assembly (AIA) views the lower atmosphere of the Sun in ultraviolet wavelengths where we can see hot plasma moving along magnetic field lines. Home page for the Atmospheric Imaging Assembly.

SDO Helioseismic Magnetic Imager (HMI) Continuum Images

The continuum images are constructed from several filters on HMI which closely resemble an optical image.

The Helioseismic and Magnetic Imager (HMI) images the Sun in a set of narrow wavelengths which enables us to study motions at the solar surface and collect magnetic field information. Home Page for the Helioseismic and Magnetic Imager.

SDO HMI Magnetograms

Magnetograms are constructed from multiple images, measuring the splitting of spectral lines in a magnetic field, called the Zeeman effect (Wikipedia).

The Helioseismic and Magnetic Imager (HMI) images the Sun in a set of narrow wavelengths which enables us to study motions at the solar surface and collect magnetic field information. Home Page for the Helioseismic and Magnetic Imager.

  • Full Disk View - March 29, 2010
    2010.04.21
    This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Grey is zero magnetic field.

    The black and white region slightly above the center corresponds to a visible sunspot. Weaker magnetic regions are visible around the disk.

  • Sunspot Close-Up - March 29, 2010
    2010.04.21
    This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Grey is zero magnetic field.

    This version is a close-up view of a large sunspot group.

  • Sunspot Zoom-In - March 29, 2010
    2010.04.21
    This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Grey is zero magnetic field.

    This movie zooms-in on a large sunspot group.

  • Full Disk View - April 7, 2010
    2010.04.21
    This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Grey is zero magnetic field.

    Notice that the surface magnetic fields reveal much more structure than the white-light images in

    SDO/HMI Continuum Full Disk View - April 7, 2010

SDO HMI Dopplergrams

Dopplergrams are also constructed from multiple filtered images, measuring the speed of each pixel by measuring the Doppler Shift (Wikipedia) of the spectral line.

The Helioseismic and Magnetic Imager (HMI) images the Sun in a set of narrow wavelengths which enables us to study motions at the solar surface and collect magnetic field information. Home Page for the Helioseismic and Magnetic Imager.

  • Sunspot Close-Up - March 29, 2010
    2010.04.21
    The dopplergram from SDO/HMI data shows the velocity of solar material on the line-of-sight. White pixels are moving away from the camera and black pixels are moving towards the camera.

SDO and Previous Missions

  • SDO and SOHO
    2010.03.31
    This movie compares the spatial and temporal resolutions of the SDO/AIA (Atmospheric Imaging Assembly) imager to the SOHO/EIT (Extreme ultraviolet Imaging Telescope) imager. SOHO/EIT's highest resolution is 1024x1024 pixels with images taken about every 12 minutes for the 195 Ångstrom band. The SDO/AIA 193 band takes images at 4096x4096 pixels every twelve seconds!

    In this movie we can see the difference this makes for a closeup view of Active Region 1087. EIT reveals changes in the active region, which AIA reveals many details.

    This visualization is a companion piece to A Comparative View of the Sun: SDO/AIA 193 and STEREO-B/EUVI 195.

  • SDO and STEREO
    2010.03.24
    This movie compares the spatial and temporal resolutions of the SDO/AIA (Atmospheric Imaging Assembly) imager to the STEREO/EUVI (Extreme UltraViolet Imager) imager. STEREO-B/EUVI's highest resolution is 2048x2048 pixels with images taken about every 5 minutes for the 195 Ångstrom band. The SDO/AIA 193 band takes images at 4096x4096 pixels every twelve seconds!

    While STEREO's vantage point at this time is very different from SDO, we can still identify some features of the Active Region 1087 in these two views. EUVI shows the launch of the filament, while AIA reveals many finer details.

    This visualization is a companion piece to A Comparative View of the Sun: SDO/AIA 193 and SOHO/EIT 195.

Additional SDO Resources

  • SDO Pre-Launch
    List
    A variety of movies assembled from prior missions as a prelude to SDO.
  • SDO - Edited Features
    List
    Views of the instruments, interviews with scientists and engineers, and other goodies.
  • SDO on YouTube
    External Resource
    A collection of videos from the press conference.
  • SDO First Light High Resolution Stills
    2010.04.28
    Stills from the AIA instrument on SDO. They show the March 30, 2010 "First Light" prominence eruption captured just after the AIA sensors were activated. All images are from the ultraviolet part of the spectrum, specifically the wavelengths of 304, 211, 193, and 171 Ångstroms. The stills are in multiple resolutions and are available as tiff and jpeg files.