SDO HMI 2014-12-06 19:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.46 | 0.00 | 10.56 | 14.19 | 17.90 | -6.12 | 1.96 | 0.2679 | -714.8 | -588.5 | |
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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 | 1.19 | 0.00 | 0.61 | 14.91 | 24.52 | 0.50 | 358.09 | 0.2555 | -898.0 | -799.6 | |
| 0.00 | 2.56 | 0.00 | 1.30 | 12.33 | 21.52 | -2.50 | 11.44 | 0.2157 | -730.0 | -639.7 | |
| 0.00 | 2.64 | 0.00 | 1.32 | 8.58 | 21.33 | -2.68 | 17.58 | 0.1539 | -882.0 | -651.5 | |
| 0.00 | 0.85 | 0.00 | 0.43 | 12.88 | 21.21 | -2.81 | 12.25 | 0.2259 | -919.0 | -738.7 | |
| 0.00 | 2.30 | 0.00 | 1.19 | 15.62 | 18.93 | -5.08 | 17.77 | 0.2807 | -732.0 | -581.0 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 13.67 | 18.95 | -5.07 | 20.21 | 0.2496 | -896.0 | -641.5 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 13.27 | 18.22 | -5.79 | 23.44 | 0.2480 | -754.0 | -683.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 18.62 | 17.95 | -6.07 | 17.58 | 0.3331 | -729.0 | -532.4 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 9.57 | 17.54 | -6.47 | 34.27 | 0.1983 | -914.0 | -743.6 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 13.28 | 17.25 | -6.77 | 26.86 | 0.2550 | -869.0 | -652.7 | |
| 0.00 | 0.77 | 0.00 | 0.39 | 12.22 | 16.91 | -7.11 | 30.11 | 0.2421 | -837.0 | -678.6 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 20.31 | 15.63 | -8.38 | 21.67 | 0.3719 | -799.0 | -569.8 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 15.66 | 13.52 | -10.50 | 33.33 | 0.3207 | -777.0 | -615.4 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 15.56 | 13.30 | -10.71 | 34.02 | 0.3215 | -750.0 | -728.2 | |
| 0.00 | 0.94 | 0.00 | 0.56 | 24.15 | 359.26 | -24.76 | 43.24 | 0.5600 | 764.0 | 573.5 | |
| 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. | |