| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.10 | 229.68 | 23.44 | 119.36 | 17.71 | 223.44 | 6.71 | 338.34 | 0.3035 | -700.1 | -384.7 | |
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back to the solar disc SDO HMI 2011-11-27 03:58:57 UT
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| 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 | 18.82 | 224.99 | 8.26 | 335.57 | 0.3302 | 832.0 | 639.3 | |
| 15.06 | 83.61 | 7.82 | 43.39 | 17.38 | 224.05 | 7.32 | 336.16 | 0.3021 | -1257.4 | -511.1 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.81 | 224.07 | 7.33 | 336.71 | 0.3087 | -262.0 | -246.4 | |
| 28.50 | 117.07 | 14.81 | 60.91 | 17.84 | 223.41 | 6.68 | 338.62 | 0.3051 | -1300.5 | -375.6 | |
| 1.28 | 1.88 | 0.68 | 0.99 | 20.14 | 223.50 | 6.77 | 340.97 | 0.3411 | 836.7 | 797.6 | |
| 0.26 | -4.00 | 0.13 | -4.00 | 18.24 | 223.27 | 6.54 | 339.52 | 0.3104 | -760.0 | 999999 | |
| 0.00 | 2.74 | 0.00 | 1.40 | 14.99 | 222.17 | 5.44 | 338.69 | 0.2532 | 975.0 | 735.2 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 19.80 | 221.94 | 5.21 | 344.84 | 0.3282 | -871.0 | -728.0 | |
| 0.00 | 9.07 | 0.00 | 4.71 | 18.21 | 221.86 | 5.13 | 343.63 | 0.3026 | -847.0 | -806.4 | |
| 0.00 | 2.14 | 0.00 | 1.10 | 15.63 | 221.76 | 5.03 | 341.04 | 0.2609 | 912.0 | 725.6 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 15.18 | 221.68 | 4.95 | 340.69 | 0.2532 | 1063.0 | 827.1 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 19.89 | 221.53 | 4.80 | 346.05 | 0.3280 | -907.0 | -759.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.57 | 221.42 | 4.69 | 342.17 | 0.2581 | 912.0 | 726.2 | |
| 0.00 | 1.88 | 0.00 | 0.98 | 19.42 | 221.36 | 4.63 | 346.17 | 0.3198 | -1031.0 | -841.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 16.43 | 220.45 | 3.72 | 346.50 | 0.2676 | 920.0 | 700.8 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 17.05 | 219.69 | 2.95 | 349.63 | 0.2751 | 699.0 | 585.5 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 23.94 | 218.66 | 1.92 | 355.42 | 0.3859 | 775.0 | 608.7 | |
| 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. | |