| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.80 | 429.82 | 35.65 | 222.92 | 16.04 | 64.42 | 11.61 | 319.15 | 0.2972 | -1115.3 | -446.3 | |
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back to the solar disc SDO HMI 2011-11-12 06:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 0.87 | 17.16 | 70.14 | 17.32 | 310.58 | 0.3762 | -632.0 | -529.8 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 18.60 | 66.10 | 13.28 | 320.81 | 0.3460 | -660.0 | -520.1 | |
| 65.27 | 404.31 | 33.85 | 209.69 | 15.96 | 64.57 | 11.76 | 318.56 | 0.2973 | -1497.8 | -452.3 | |
| 0.00 | 2.33 | 0.00 | 1.22 | 18.77 | 64.73 | 11.91 | 324.06 | 0.3344 | -809.0 | -648.4 | |
| 0.00 | 6.37 | 0.00 | 3.31 | 17.25 | 63.64 | 10.82 | 323.64 | 0.3039 | -804.0 | -744.6 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 16.76 | 63.58 | 10.76 | 322.77 | 0.2969 | -193.0 | -204.8 | |
| 0.00 | 1.98 | 0.00 | 1.03 | 17.78 | 62.72 | 9.90 | 327.02 | 0.3023 | -807.0 | -589.5 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 16.83 | 62.55 | 9.73 | 325.62 | 0.2877 | -826.0 | -637.7 | |
| 0.00 | 1.55 | 0.00 | 0.80 | 17.26 | 62.13 | 9.31 | 327.62 | 0.2898 | -991.0 | -793.7 | |
| 2.50 | 3.19 | 1.26 | 1.61 | 13.82 | 58.64 | 5.82 | 331.90 | 0.2102 | 1023.3 | 957.6 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 13.68 | 58.03 | 5.21 | 334.15 | 0.2032 | 881.0 | 661.1 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 19.10 | 57.76 | 4.95 | 343.45 | 0.2873 | 815.0 | 602.4 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 19.72 | 57.75 | 4.93 | 344.12 | 0.2971 | 996.0 | 701.1 | |
| 1.03 | 1.55 | 0.54 | 0.81 | 21.94 | 54.30 | 1.48 | 355.73 | 0.3236 | 765.6 | 678.0 | |
| 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. | |