SDO HMI 2014-11-30 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.36 | 0.00 | 11.65 | -23.03 | 92.31 | -18.46 | 144.33 | 0.5023 | -523.9 | -484.2 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.53 | -23.58 | 94.88 | -15.88 | 148.88 | 0.4872 | 784.0 | 590.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -20.62 | 94.37 | -16.39 | 144.32 | 0.4548 | -882.0 | -706.4 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -19.76 | 94.40 | -16.36 | 143.16 | 0.4441 | -667.0 | -574.9 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -24.01 | 93.17 | -17.59 | 146.81 | 0.5064 | -911.0 | -762.0 | |
| 0.00 | 4.19 | 0.00 | 2.41 | -24.05 | 92.76 | -18.01 | 146.26 | 0.5103 | -594.0 | -663.3 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -22.78 | 92.94 | -17.83 | 144.96 | 0.4936 | -686.0 | -614.3 | |
| 0.00 | 1.37 | 0.00 | 0.79 | -23.72 | 92.67 | -18.09 | 145.74 | 0.5071 | -816.0 | -660.4 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -23.59 | 92.59 | -18.18 | 145.46 | 0.5063 | -678.0 | -570.8 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -24.24 | 92.49 | -18.27 | 146.11 | 0.5149 | -616.0 | -490.6 | |
| 0.00 | 1.62 | 0.00 | 0.91 | -20.66 | 91.98 | -18.78 | 140.72 | 0.4779 | -881.0 | -687.0 | |
| 0.00 | 1.28 | 0.00 | 0.72 | -20.54 | 91.79 | -18.97 | 140.27 | 0.4782 | -732.0 | -555.3 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -25.57 | 90.54 | -20.22 | 145.07 | 0.5466 | -644.0 | -555.4 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -25.17 | 90.26 | -20.50 | 144.25 | 0.5445 | -595.0 | -529.6 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -24.32 | 90.03 | -20.73 | 142.91 | 0.5371 | -677.0 | -540.7 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -20.45 | 90.60 | -20.16 | 138.47 | 0.4892 | 736.0 | 604.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |