SDO HMI 2014-11-08 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.21 | 21.75 | 0.70 | 12.32 | 5.26 | 72.60 | 29.10 | 274.27 | 0.4870 | -218.2 | -276.0 | |
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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 | 4.14 | 0.00 | 2.42 | 5.56 | 75.75 | 32.24 | 274.61 | 0.5348 | -907.0 | -730.7 | |
| 0.69 | 2.33 | 0.40 | 1.35 | 5.27 | 74.85 | 31.34 | 274.10 | 0.5214 | -818.0 | -684.1 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 4.54 | 74.46 | 30.95 | 272.69 | 0.5154 | -733.0 | -590.4 | |
| 0.00 | 1.04 | 0.00 | 0.59 | 5.18 | 73.80 | 30.29 | 273.99 | 0.5056 | -669.0 | -507.4 | |
| 0.00 | 1.04 | 0.00 | 0.59 | 4.12 | 73.71 | 30.21 | 271.87 | 0.5041 | -631.0 | -511.4 | |
| 0.52 | 3.02 | 0.30 | 1.72 | 5.20 | 73.39 | 29.88 | 274.04 | 0.4994 | -839.8 | -759.3 | |
| 0.00 | 1.55 | 0.00 | 0.88 | 5.06 | 73.21 | 29.70 | 273.76 | 0.4966 | -881.0 | -756.8 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 5.10 | 72.69 | 29.19 | 273.88 | 0.4889 | -738.0 | -582.7 | |
| 0.00 | 2.07 | 0.00 | 1.16 | 5.91 | 71.61 | 28.11 | 275.66 | 0.4729 | 878.0 | 737.8 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 5.68 | 67.35 | 23.84 | 275.73 | 0.4060 | 528.0 | 478.9 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 3.56 | 66.52 | 23.01 | 270.44 | 0.3919 | 738.0 | 526.9 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 5.73 | 66.53 | 23.03 | 275.99 | 0.3931 | 828.0 | 724.3 | |
| 0.00 | 1.47 | 0.00 | 0.79 | 6.33 | 66.43 | 22.93 | 277.54 | 0.3922 | 835.0 | 673.9 | |
| 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. | |