Ten Years of Solar Dynamics Observatory
- Visualizations by:
- Tom Bridgman
- Written by:
- Mara Johnson-Groh
- Scientific consulting by:
- William D. Pesnell
- Produced by:
- Scott Wiessinger
- View full credits
Here we present a continuous run of data from the AIA instrument 171 angstrom filter aboard Solar Dynamics Observatory (SDO). Compiling one photo every hour, the movie condenses a decade of the Sun (June 2, 2010-June 1, 2020) into an almost 49 minute time lapse, where every second corresponds to 30 hours of SDO data.
There's a number of phenomema observed:
Naturally this movie includes a number of events that have been explored previously:
Interesting physical features:
At various times the AIA instrument failed to collect data resulting in some large data gaps appearing in this visualization as black frames.
There's a number of phenomema observed:
- Earth eclipses: usually occur in February-March and August-September each year.
- Lunar transits: We see the lunar disk block out the Sun
- Instrument repointings for calibration purposes
Naturally this movie includes a number of events that have been explored previously:
- October 7, 2010: Lunar Transit
- February 24, 2011: Trebuchet eruption
- June 7, 2011: Massive eruption
- December 15, 2011: Comet Lovejoy
- June 6, 2012: Venus Transit 2012 (raw content)
- July 19, 2012: Raining Loops
- August 31, 2012: Magnificent CME
- September 29, 2013: Canyon of Fire
- October 23-28, 2013: Five days of flares and CMEs
- April 2, 2014: Graceful eruption
- July 8, 2014: Firework flare
- October 2, 2014: Mid-level flare and eruption
- October 8, 2014: Pumpkin Sun
- October 19-27 2014: Giant sunspot flares
- December 19, 2014: Holiday Lights
- April 21, 2015: Phoenix Prominence Eruption
- June 18, 2015: Arching Eruption
- May 9, 2016: Mercury transit 2016 (raw content))
- July 5, 2017: Life of Sunspot
- September 6, 2017: September flares (biggest)
- November 11, 2019: Mercury Transit 2019 (raw content)
Interesting physical features:
- In October and November 2014, a large helmet streamer is visible extremely high above the solar limb. You can still observe it above the solar limb as it moves across the far-side of the Sun.
At various times the AIA instrument failed to collect data resulting in some large data gaps appearing in this visualization as black frames.
- April 1, 2015: about 8 hours
- May 13, 2015: about 6 hours
- December 26, 2015: about 27 hours
- August 2, 2016: about 8 days
- April 30, 2017: about a day
- June 28, 2018: about 18 hours
Credits
Please give credit for this item to:
NASA's Scientific Visualization Studio
Visualizer
- Tom Bridgman (GST) [Lead]
Writer
- Mara Johnson-Groh (Wyle Information Systems) [Lead]
Scientist
- William D. Pesnell (NASA/GSFC) [Lead]
Producer
- Scott Wiessinger (KBRwyle) [Lead]
Technical support
- Ian Jones (ADNET)
- Laurence Schuler (ADNET)
Missions
This visualization is related to the following missions:Datasets used in this visualization
SDO AIA 171 (A.K.A. 171 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER
Dataset can be found at: http://jsoc.stanford.edu/
See more visualizations using this data setHEK (A.K.A. Heliophysics Event Knowledgebase)
Event List
|
LMSAL
Heliophysics Event Knowledgebase
See more visualizations using this data setSolar Dynamics Observatory Spacecraft Operations (A.K.A. Spacecraft Events)
Event List
|
JSOC
SDO Events Calendar
See more visualizations using this data setNote: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.
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