SDO HMI 2011-11-25 06:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.52 | 52.15 | 9.63 | 30.22 | -15.87 | 267.48 | 26.03 | 234.78 | 0.5201 | 497.8 | 393.3 | |
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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 | 0.69 | 0.00 | 0.40 | -11.84 | 269.52 | 28.07 | 243.47 | 0.5169 | 680.0 | 567.0 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -12.30 | 269.44 | 27.99 | 242.60 | 0.5185 | 637.0 | 559.8 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -12.26 | 268.85 | 27.40 | 242.19 | 0.5105 | 813.0 | 707.0 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -17.45 | 269.30 | 27.85 | 233.98 | 0.5531 | 722.0 | 555.4 | |
| 0.00 | 2.74 | 0.00 | 1.57 | -12.49 | 268.03 | 26.58 | 241.08 | 0.5010 | 692.0 | 570.5 | |
| 0.94 | 5.05 | 0.54 | 2.88 | -12.15 | 267.89 | 26.44 | 241.57 | 0.4969 | 998.6 | 724.8 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -12.27 | 267.67 | 26.21 | 241.16 | 0.4948 | 789.0 | 613.6 | |
| 9.16 | 32.20 | 5.35 | 18.78 | -16.99 | 267.80 | 26.35 | 233.27 | 0.5317 | 966.9 | 501.5 | |
| 6.42 | -8.00 | 3.74 | -8.00 | -16.65 | 267.64 | 26.19 | 233.66 | 0.5271 | 943.5 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -13.36 | 266.81 | 25.35 | 238.40 | 0.4912 | 668.0 | 436.4 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -17.65 | 265.70 | 24.25 | 230.02 | 0.5128 | -726.0 | -590.7 | |
| 0.00 | 0.34 | 0.00 | 0.20 | -17.96 | 265.10 | 23.64 | 228.86 | 0.5086 | -751.0 | -744.0 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -18.99 | 264.53 | 23.08 | 226.62 | 0.5121 | -480.0 | -411.6 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -19.27 | 263.96 | 22.51 | 225.51 | 0.5086 | -654.0 | -487.2 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -18.41 | 260.60 | 19.15 | 222.35 | 0.4640 | -864.0 | -653.6 | |
| 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. | |