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@ -140,7 +140,7 @@ When checked, displays imagary from NASA's SDO (Solar Dynamic Observatory) and E
SDOs images the Sun in a variety of UV and EUV wavelengths. SOHO shows images of the solar corona. The images are near real-time, updated every 15 minutes. SDOs images the Sun in a variety of UV and EUV wavelengths. SOHO shows images of the solar corona. The images are near real-time, updated every 15 minutes.
Solar flares are particularly visible in the AIA 131 Å images. Solar flares are particularly visible in the AIA 131 Å images.
<h3>18: Image or Video Selection</h3> <h3>18: Image or Video Selection</h3>
@ -150,24 +150,24 @@ Selects whether to display images (unchecked) or video (checked).
Selects which image / wavelength to view. Selects which image / wavelength to view.
* AIA 94 Å to 1700 Å - The AIA (Atmospheric Imaging Assembly) images the solar atmosphere at multiple EUV (Extreme Ultraviolet) and UV (Ultraviolet) wavelengths: * AIA 94 Å to 1700 Å - The AIA (Atmospheric Imaging Assembly) images the solar atmosphere at multiple EUV (Extreme Ultraviolet) and UV (Ultraviolet) wavelengths:
| Band | Region | | Band | Region |
|---------|-----------------------------------------| |---------|-----------------------------------------|
| 94 Å | Flaring | | 94 Å | Flaring |
| 131 Å | Flaring | | 131 Å | Flaring |
| 171 Å | Quiet corona, upper transition region | | 171 Å | Quiet corona, upper transition region |
| 193 Å | Corona and hot flare plasma | | 193 Å | Corona and hot flare plasma |
| 211 Å | Active corona | | 211 Å | Active corona |
| 304 Å | Chromosphere, transition region | | 304 Å | Chromosphere, transition region |
| 335 Å | Active corona | | 335 Å | Active corona |
| 1600 Å | Transition region, upper photoshere | | 1600 Å | Transition region, upper photoshere |
| 1700 Å | Temperature minimum, photosphere | | 1700 Å | Temperature minimum, photosphere |
[Ref](https://sdo.gsfc.nasa.gov/data/channels.php) [Ref](https://sdo.gsfc.nasa.gov/data/channels.php)
* MHI Magnetogram - HMI (Helioseismic and Magnetic Imager) Magnetogram shows the magnetic field in the photosphere, with black and white indicating opposite polarities. * MHI Magnetogram - HMI (Helioseismic and Magnetic Imager) Magnetogram shows the magnetic field in the photosphere, with black and white indicating opposite polarities.
* MHI Intensitygram - Brightness in a visible light band (6173 Å - Red - Iron spectral line), useful for observing sun spots. * MHI Intensitygram - Brightness in a visible light band (6173 Å - Red - Iron spectral line), useful for observing sun spots.
* Dopplergram - Shows velocities along the line-of-sight. * Dopplergram - Shows velocities along the line-of-sight.
* LASCO (Large Angle Spectrometric Coronagraph) shows solar corona. C2 shows corona up to 8.4Mkm. C3 shows corona up to 23Mkm. * LASCO (Large Angle Spectrometric Coronagraph) shows solar corona. C2 shows corona up to 8.4Mkm. C3 shows corona up to 23Mkm.