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