From 8711f77fdbbc4da95c6b7a36038a00d2ba7cb7ab Mon Sep 17 00:00:00 2001 From: Daniele Forsi Date: Sat, 6 Apr 2024 12:22:46 +0200 Subject: [PATCH] Convert encoding from ISO-8859-1 to UTF-8 --- plugins/feature/sid/readme.md | 24 ++++++++++++------------ 1 file changed, 12 insertions(+), 12 deletions(-) diff --git a/plugins/feature/sid/readme.md b/plugins/feature/sid/readme.md index 3796d8920..2f87dd95a 100644 --- a/plugins/feature/sid/readme.md +++ b/plugins/feature/sid/readme.md @@ -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. -Solar flares are particularly visible in the AIA 131 Å images. +Solar flares are particularly visible in the AIA 131 Ã… images.

18: Image or Video Selection

@@ -150,24 +150,24 @@ Selects whether to display images (unchecked) or video (checked). 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 Ã… to 1700 Ã… - The AIA (Atmospheric Imaging Assembly) images the solar atmosphere at multiple EUV (Extreme Ultraviolet) and UV (Ultraviolet) wavelengths: | Band | Region | |---------|-----------------------------------------| -| 94 Å | Flaring | -| 131 Å | Flaring | -| 171 Å | Quiet corona, upper transition region | -| 193 Å | Corona and hot flare plasma | -| 211 Å | Active corona | -| 304 Å | Chromosphere, transition region | -| 335 Å | Active corona | -| 1600 Å | Transition region, upper photoshere | -| 1700 Å | Temperature minimum, photosphere | +| 94 Ã… | Flaring | +| 131 Ã… | Flaring | +| 171 Ã… | Quiet corona, upper transition region | +| 193 Ã… | Corona and hot flare plasma | +| 211 Ã… | Active corona | +| 304 Ã… | Chromosphere, transition region | +| 335 Ã… | Active corona | +| 1600 Ã… | Transition region, upper photoshere | +| 1700 Ã… | Temperature minimum, photosphere | [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 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 Ã… - Red - Iron spectral line), useful for observing sun spots. * 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.