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Sun In Time:
Please note: A cooling water line burst in the Stanford building housing
the pipeline servers for SDO/HMI and SDO/AIA on 2024-11-26. Currently,
these data servers are offline while the damage is assessed and
repaired. This means that all HMI and AIA data will be unavailable until
repairs are completed and the pipeline is restarted, and thus no data
from HMI and AIA since 2024-11-26 will show on this webpage until that
time. The data servers are likely to be offline for an extended interval
of time. We appreciate your understanding. More information may be found
here. (This
message was originally posted 2024-11-28, and updated on 2024-12-03.)
Image Channels
304 |
1600 |
1700 |
304-211-171
094-335-193 |
094 |
335 |
131
211-193-171 |
211 |
193 |
171
HMI cont |
HMI B(los) |
171-B(los)
Tip: Hover over the wavelength labels underneath the set of images to change the thumbnail image.
Movie links:
Daily movies:
Not Yet Available
304‑211‑171 |
94‑335‑193 |
211‑193‑171 |
171‑B(los)
Other resources:
Image data request form:
click here
SolarMonitor for this date:
click here
IRIS pointing summary for this date:
click here
Not Available
Interactive PFSS model for this date:
click here
STEREO Science Center daily browse data for this date:
click here
AIA emission measure data:
click here (image) or
click here (movie) or
click here (genx cube) or
click here (source code)
Rights/Usage
Images and movies from the Solar Dynamics Observatory (SDO) are not
copyrighted unless explicitly noted. The use of SDO images for
non-commercial purposes and public education and information efforts is
strongly encouraged and requires no expressed authorization. It is
requested, however, that any such use properly attributes the source of
the images, movies, or derived data products (as appropriate) with a
statement such as:
SDO images and movies displayed on this webpage are courtesy of NASA, and the respective AIA and HMI science teams at Lockheed Martin and at Stanford University. The coronal magnetic field visualizations are based on the models described in Schrijver & DeRosa, "Photospheric and Heliospheric Magnetic Fields", which was published in the journal Solar Physics in 2003. Emission measure data are based on the method described in Cheung et al., "Thermal Diagnostics with the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory: A Validated Method for Differential Emission Measure Inversions", which was published in The Astrophysical Journal in 2015.