SDO HMI 2011-11-30 13:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 96.97 | 411.19 | 66.39 | 280.09 | 8.02 | 128.87 | -42.86 | 79.32 | 0.6867 | -1.0 | 0.8 | |
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back to the solar disc SDO HMI 2011-11-30 13:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.30 | 151.13 | 18.79 | 96.75 | 7.49 | 132.70 | -39.03 | 79.39 | 0.6375 | -1046.0 | -396.6 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 4.22 | 132.21 | -39.52 | 84.58 | 0.6398 | -732.0 | -630.4 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 5.10 | 132.03 | -39.70 | 83.22 | 0.6430 | -682.0 | -536.2 | |
| 0.00 | 1.03 | 0.00 | 0.66 | 5.46 | 131.85 | -39.88 | 82.69 | 0.6458 | -634.0 | -544.6 | |
| 3.08 | 10.00 | 2.00 | 6.50 | 6.61 | 131.59 | -40.14 | 80.95 | 0.6508 | -882.1 | -719.6 | |
| 0.00 | 1.96 | 0.00 | 1.28 | 5.34 | 131.59 | -40.14 | 82.91 | 0.6492 | -562.0 | -465.6 | |
| 5.89 | 9.91 | 3.86 | 6.48 | 7.03 | 131.27 | -40.46 | 80.37 | 0.6555 | -808.0 | -634.4 | |
| 0.00 | 0.94 | 0.00 | 0.61 | 6.61 | 131.32 | -40.41 | 81.00 | 0.6544 | -502.0 | -406.3 | |
| 0.00 | 1.03 | 0.00 | 0.67 | 6.81 | 130.90 | -40.83 | 80.76 | 0.6600 | -432.0 | -387.8 | |
| 0.00 | 3.16 | 0.00 | 2.09 | 7.14 | 130.47 | -41.26 | 80.35 | 0.6661 | -766.0 | -573.9 | |
| 1.28 | 1.45 | 0.86 | 0.97 | 7.43 | 129.72 | -42.01 | 80.05 | 0.6762 | -489.8 | -712.5 | |
| 0.00 | 0.85 | 0.00 | 0.57 | 7.72 | 129.64 | -42.09 | 79.62 | 0.6776 | 440.0 | 330.3 | |
| 0.00 | 1.28 | 0.00 | 0.86 | 7.54 | 129.54 | -42.19 | 79.91 | 0.6786 | -495.0 | -411.7 | |
| 0.00 | 2.31 | 0.00 | 1.56 | 7.69 | 129.28 | -42.45 | 79.74 | 0.6821 | -617.0 | -526.7 | |
| 0.00 | 1.54 | 0.00 | 1.04 | 7.74 | 128.99 | -42.74 | 79.71 | 0.6858 | -678.0 | -516.3 | |
| 0.00 | 0.68 | 0.00 | 0.46 | 7.33 | 128.84 | -42.89 | 80.34 | 0.6871 | -529.0 | -438.2 | |
| 0.00 | 2.90 | 0.00 | 1.99 | 7.26 | 128.44 | -43.29 | 80.50 | 0.6921 | -633.0 | -538.7 | |
| 0.00 | 1.28 | 0.00 | 0.88 | 7.34 | 127.89 | -43.84 | 80.46 | 0.6990 | -487.0 | -408.3 | |
| 0.00 | 1.20 | 0.00 | 0.83 | 7.43 | 127.67 | -44.06 | 80.37 | 0.7018 | -385.0 | -345.0 | |
| 2.14 | 197.94 | 1.50 | 140.86 | 9.49 | 127.29 | -44.44 | 77.54 | 0.7096 | -381.8 | 383.4 | |
| 4.78 | -20.00 | 3.35 | -20.00 | 9.25 | 127.20 | -44.53 | 77.89 | 0.7103 | -280.3 | 999999 | |
| 3.50 | -20.00 | 2.45 | -20.00 | 8.89 | 127.21 | -44.52 | 78.39 | 0.7095 | 853.0 | 999999 | |
| 0.26 | -20.00 | 0.18 | -20.00 | 9.16 | 127.17 | -44.56 | 78.02 | 0.7105 | 160.3 | 999999 | |
| 2.31 | -20.00 | 1.62 | -20.00 | 8.50 | 126.98 | -44.75 | 78.98 | 0.7117 | 923.3 | 999999 | |
| 1.03 | -20.00 | 0.72 | -20.00 | 7.98 | 126.54 | -45.19 | 79.77 | 0.7162 | 714.0 | 999999 | |
| 38.36 | -20.00 | 27.39 | -20.00 | 8.43 | 126.05 | -45.68 | 79.23 | 0.7227 | 942.7 | 999999 | |
| 1.11 | -20.00 | 0.80 | -20.00 | 7.97 | 125.56 | -46.17 | 79.93 | 0.7280 | 565.9 | 999999 | |
| 2.90 | 7.86 | 2.12 | 5.73 | 10.09 | 125.16 | -46.57 | 77.12 | 0.7358 | 734.6 | 549.6 | |
| 0.00 | 1.11 | 0.00 | 0.80 | 7.53 | 125.54 | -46.19 | 80.55 | 0.7277 | -7.0 | -41.2 | |
| 0.00 | 1.62 | 0.00 | 1.18 | 9.61 | 125.16 | -46.57 | 77.77 | 0.7350 | 672.0 | 618.6 | |
| 0.00 | 0.94 | 0.00 | 0.69 | 9.76 | 124.96 | -46.77 | 77.61 | 0.7376 | 534.0 | 448.8 | |
| 1.03 | 1.54 | 0.75 | 1.12 | 7.72 | 124.77 | -46.96 | 80.39 | 0.7369 | 465.8 | 463.3 | |
| 0.00 | 2.14 | 0.00 | 1.62 | 7.31 | 122.63 | -49.10 | 81.20 | 0.7609 | 474.0 | 316.2 | |
| 0.00 | 1.03 | 0.00 | 0.81 | 5.71 | 120.94 | -50.78 | 83.44 | 0.7783 | -555.0 | -500.4 | |
| 0.00 | 1.71 | 0.00 | 1.37 | 6.62 | 120.15 | -51.58 | 82.34 | 0.7875 | 490.0 | 371.1 | |
| 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. | |