SDO
Solar Dynamics Observatory
First mission in NASA's Living With a Star (LWS) program. Initially planned for
launch in early 2009.
SDO will help understand how the Sun's magnetic field is generated and
structured and how this magnetic energy is converted into solar wind and
energetic particles.
http://sdo.gsfc.nasa.gov/
Prime
contractor
|
Lockheed
Martin
|
Platform
|
|
Mass
at launch
|
3100
kg
|
Dry
mass
|
1650
kg
|
Dimension
|
2.2
x 2.2 x 4.5 m
|
Solar
array
|
|
Stabilization
|
3-axis
|
DC
power
|
1450
W
|
Design
lifetime
|
|
Downlink in Ka-band at 130 Mbps (continuous)
HMI (Helioseismic and Magnetic Imager)
Will extend the capabilities of the SOHO/MDI instrument with continuous
full-disk coverage at higher spatial resolution. Provided by Stanford
University. Will study the origin of solar variability and attempt to
characterise and understand the Sun's interior and magnetic activity.
AIA (Atmospheric Imaging Assembly)
Will image the solar atmosphere in multiple wavelengths to link changes
in the surface to interior changes. Data will include images of the Sun in 10
wavelengths every 10 seconds. Provided by Lockheed Martin Solar Astrophysics
Laboratory. Composed of 4 telescopes.
EVE (Extreme Ultraviolet Variablity Experiment)
Will measure the solar extreme-ultraviolet (EUV) irradiance with
unprecedented spectral resolution, temporal cadence, and precision. Measures
the solar extreme ultraviolet (EUV, ranges in wavelength from 0.1 to 105 nm)
spectral irradiance to understand variations on the timescales which influence
Earth's climate and near-Earth space. Provided by University of Colorado.