SDO HMI 2011-11-23 20:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.98 | 80.31 | 9.48 | 42.23 | -16.85 | 265.98 | 5.85 | 196.92 | 0.3385 | 47.3 | -107.9 | |
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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 | 0.49 | -11.86 | 268.87 | 8.75 | 212.19 | 0.2808 | 947.0 | 708.3 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -12.34 | 268.34 | 8.22 | 209.69 | 0.2831 | 835.0 | 665.8 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -18.42 | 268.55 | 8.43 | 201.90 | 0.3746 | 803.0 | 489.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -15.82 | 268.40 | 8.28 | 204.56 | 0.3348 | 893.0 | 734.1 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -12.58 | 267.98 | 7.86 | 208.19 | 0.2837 | 871.0 | 643.1 | |
| 14.90 | 37.16 | 7.86 | 19.61 | -16.97 | 267.61 | 7.49 | 201.14 | 0.3471 | 1152.7 | 557.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -18.63 | 266.55 | 6.43 | 196.87 | 0.3670 | 808.0 | 686.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -16.59 | 266.13 | 6.01 | 197.62 | 0.3331 | -759.0 | -589.1 | |
| 0.00 | 1.37 | 0.00 | 0.73 | -19.20 | 265.81 | 5.69 | 194.62 | 0.3726 | 742.0 | 621.0 | |
| 0.00 | 7.96 | 0.00 | 4.17 | -16.40 | 265.60 | 5.48 | 196.31 | 0.3276 | -1184.0 | -951.1 | |
| 0.00 | 2.23 | 0.00 | 1.17 | -16.77 | 265.18 | 5.05 | 194.80 | 0.3316 | -738.0 | -593.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -14.35 | 265.12 | 5.00 | 196.83 | 0.2927 | 947.0 | 664.9 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -17.14 | 264.04 | 3.92 | 191.34 | 0.3333 | -740.0 | -616.3 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -18.34 | 263.94 | 3.82 | 190.38 | 0.3523 | -866.0 | -738.6 | |
| 0.00 | 4.37 | 0.00 | 2.29 | -17.18 | 263.70 | 3.57 | 190.36 | 0.3328 | -1156.0 | -912.2 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -17.30 | 263.45 | 3.33 | 189.60 | 0.3341 | -928.0 | -732.5 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -18.24 | 263.47 | 3.35 | 189.17 | 0.3494 | -638.0 | -631.9 | |
| 3.08 | 6.42 | 1.62 | 3.37 | -16.99 | 263.42 | 3.29 | 189.66 | 0.3289 | -1080.1 | -874.7 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -16.18 | 263.37 | 3.25 | 189.97 | 0.3155 | -775.0 | -707.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -17.49 | 263.27 | 3.15 | 188.98 | 0.3367 | -592.0 | -533.0 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -16.92 | 263.17 | 3.04 | 188.97 | 0.3272 | -922.0 | -698.1 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -20.34 | 262.98 | 2.85 | 187.05 | 0.3821 | -751.0 | -634.0 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -19.22 | 262.67 | 2.55 | 186.67 | 0.3635 | -691.0 | -568.1 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -18.30 | 262.29 | 2.16 | 185.94 | 0.3479 | -941.0 | -691.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -15.55 | 256.63 | -3.49 | 168.90 | 0.3061 | -940.0 | -678.7 | |
| 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. | |