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Solar Activity
Corona Holes
Coronal Properties
Cosmic Rays
Solar Active Regions
Solar Events
Solar Flares
Solar Imagery
Solar Irradiance
Solar Prominences
Solar Radio Waves
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GCMD >> EARTH SCIENCE >> Sun-earth Interactions >> Solar Activity
Movie ID Title
A short movie of the Sun around the time of maximum solar activity. 3549 Comparison: Solar Maximum from SOHO/EIT
This is a short movie of the Sun in ultraviolet light at solar minimum. 3548 Comparison: Solar Minimum from SOHO/EIT
This movie plays nearly two weeks of SOHO/EIT and SOHO/LASCO imagery from around Halloween 2003. 3504 Halloween 2003 Solar Storms: SOHO/EIT and SOHO/LASCO
This movie displays nearly two weeks of MDI magnetogram data from around Halloween 2003. 3503 Halloween 2003 Solar Storms: SOHO/MDI Magnetograms
This movie displays nearly two weeks of MDI continuum data from around Halloween 2003. 3502 Halloween 2003 Solar Storms: SOHO/MDI Continuum
This movie displays nearly two weeks of EIT 304 Ångstrom data from around Halloween 2003. 3501 Halloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 304 Å
This movie displays nearly two weeks of EIT 195 Ångstrom data from around Halloween, 2003. 3500 Halloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 195 Å
This version of the movie includes <b>ALL</b> TRACE data frames, including cases where the spacecraft re-points for short times. This makes the movie jump around considerably more than the 'smooth' version. 3435 Solar Dynamics Observatory (SDO): Data Collection Comparison
Still image showing the CME in eruption and the radio-loud component of the emission, the bright yellow-orange band between 0.2-1.0 MHz. 3432 Coronal Mass Ejections (CME): Radio Loud Variety
Still image showing the CME in eruption. The radio-loud component is not visible (between 0.2-1.0 MHz). 3431 Coronal Mass Ejections (CME): Radio Quiet Variety
This is a stereographic version of the movie. Red/Cyan stereo glasses are required to view it properly. <img src='/images/stereoicon.png'>' 3427 First 3-D Stereo from STEREO: EUVI 171 Ångstroms (South Pole View)
We begin our flight through the loops, noting that the more prominent regions on the surface have a higher density of field lines. 3346 Grand Tour of the Coronal Loops Model
Another angle of the model showing a number of active regions. 3287 Rotating Tour of Solar Coronal Loops
We pass over another group of active regions. 3286 Flight through the Coronal Loops
The PFSS model is a poor match for the TRACE coronal loops. 3212 Space Weather Forecasting: Active Times Ahead
In this case, we see the PFSS model matches the TRACE coronal loops very well. 3211 Space Weather Forecasting: Quiet Times Ahead
This short video gives an overview of NASA's SDO spacecraft mission to observe the Sun and improve predictions of solar weather. 10188 NASA's SDO Mission

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