SDO/HMI
HMI Colored
HMI Gray
HMI Flat
HMI Colored 2
Magnetogram Colorized
Magnetogram BW
SDO/AIA
AIA 094
AIA 131
AIA 171
AIA 193
AIA 211
AIA 304
AIA 335
AIA 1600
AIA 1700
171/193/211
94/193/335
171/211/304
The Solar Dynamics Observatory (SDO)

The Solar Dynamics Observatory is the first mission to be launched for NASA's Living With a Star (LWS) Program, a program designed to understand the causes of solar variability and its impacts on Earth. SDO is designed to help us understand the Sun's influence on Earth and Near-Earth space by studying the solar atmosphere on small scales of space and time and in many wavelengths simultaneously. SDO will study how solar activity is created and how Space Weather comes from that activity. Measurements of the interior of the Sun, the Sun's magnetic field, the hot plasma of the solar corona, and the irradiance that creates the ionospheres of the planets are our primary data products.

AIA (Atmospheric Imaging Assembly)
Provides full-disk imaging of the Sun in ten white light, ultraviolet and extreme ultraviolet (EUV) band passes at high spatial and temporal resolution.

HMI (Helioseismic and Magnetic Imager)
Studies solar variability and characterizes the Sun's interior and the various components of magnetic activity. HMI produces data to determine the interior sources and mechanisms of solar variability and how the physical processes inside the Sun are related to surface magnetic field and activity. It also produces data to enable estimates of the coronal magnetic field for studies of variability in the extended solar atmosphere. HMI observations will enable establishing the relationships between the internal dynamics and magnetic activity in order to understand solar variability and its effects.

EVE (Extreme Ultraviolet Variability Experiment)
Will measure the Sun's extreme ultraviolet irradiance with improved spectral resolution, "temporal cadence", accuracy, and precision over preceding measurements made by TIMED SEE, SOHO, and SORCE XPS. The instrument incorporates physics-based models in order to further scientific understanding of the relationship between solar EUV variations and magnetic variation changes in the Sun. The Sun's output of energetic extreme ultraviolet photons is primarily what heats the Earth's upper atmosphere and creates the ionosphere. Solar EUV radiation output undergoes constant changes, both moment to moment and over the Sun's 11-year solar cycle, and these changes are important to understand because they have a significant impact on atmospheric heating, satellite drag, and communications system degradation, including disruption of the Global Positioning System.

Launch Date: Feb 10, 2010

SDO Website

GOES-15
Solar X-Ray Imager

STEREO
Ahead EUVI 195
Behind EUVI 195
Ahead COR2
Behind COR2
Ahead COR1
Behind COR1

LASCO
C2
C3

SPECIAL
HMI w/ Regions
Magnetogram w/ Regions
131/171 w/ Regions
AIA 304b w/ Regions
AIA 211b w/ Coronal Holes

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