SDO HMI 2014-12-06 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.66 | 319.20 | 26.24 | 183.42 | -3.68 | 0.95 | -30.19 | 97.67 | 0.5085 | 1118.1 | 372.3 | |
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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 | 1.11 | 0.00 | 0.60 | -4.33 | 7.96 | -23.19 | 101.41 | 0.4023 | 934.0 | 811.6 | |
| 0.00 | 2.05 | 0.00 | 1.14 | -4.60 | 3.95 | -27.20 | 100.42 | 0.4652 | 533.0 | 625.5 | |
| 0.00 | 0.51 | 0.00 | 0.29 | -6.11 | 3.84 | -27.31 | 103.57 | 0.4712 | 564.0 | 457.5 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -6.26 | 3.76 | -27.38 | 103.84 | 0.4728 | 873.0 | 693.2 | |
| 0.00 | 0.68 | 0.00 | 0.38 | -7.60 | 3.64 | -27.50 | 106.53 | 0.4795 | 624.0 | 539.5 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -5.40 | 3.64 | -27.50 | 102.00 | 0.4720 | 724.0 | 559.2 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -4.07 | 3.57 | -27.58 | 99.16 | 0.4697 | 789.0 | 656.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -6.35 | 2.71 | -28.43 | 103.57 | 0.4888 | -639.0 | -462.3 | |
| 45.66 | 308.52 | 26.24 | 177.41 | -3.63 | 0.87 | -30.27 | 97.55 | 0.5096 | 1335.4 | 367.2 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -4.19 | 359.64 | -31.51 | 98.35 | 0.5289 | 521.0 | 420.2 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -4.46 | 359.31 | -31.83 | 98.77 | 0.5342 | 556.0 | 348.3 | |
| 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. | |