SDO HMI 2011-11-15 06:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.11 | 189.35 | 15.67 | 117.83 | 28.38 | 41.77 | 28.50 | 316.12 | 0.6080 | -727.0 | -372.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.55 | 174.49 | 0.97 | 108.76 | 28.04 | 42.34 | 29.08 | 315.14 | 0.6104 | -925.7 | -394.9 | |
| 6.62 | -1.00 | 4.14 | -1.00 | 28.44 | 42.19 | 28.93 | 315.79 | 0.6123 | -1052.4 | 999999 | |
| 13.67 | -1.00 | 8.52 | -1.00 | 28.14 | 42.07 | 28.80 | 315.52 | 0.6086 | -1253.6 | 999999 | |
| 3.27 | -1.00 | 2.04 | -1.00 | 28.71 | 41.74 | 28.47 | 316.56 | 0.6102 | -724.2 | 999999 | |
| 0.00 | 2.41 | 0.00 | 1.51 | 29.21 | 41.62 | 28.35 | 317.30 | 0.6134 | -605.0 | -395.4 | |
| 0.00 | 2.15 | 0.00 | 1.33 | 29.01 | 40.25 | 26.98 | 318.31 | 0.5989 | -784.0 | -615.2 | |
| 0.00 | 1.63 | 0.00 | 1.01 | 30.02 | 39.62 | 26.36 | 320.18 | 0.6025 | -608.0 | -502.6 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 29.90 | 39.40 | 26.13 | 320.25 | 0.5993 | -733.0 | -658.5 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 29.64 | 38.94 | 25.68 | 320.37 | 0.5928 | -744.0 | -588.5 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 30.21 | 38.84 | 25.57 | 321.18 | 0.5973 | -694.0 | -562.8 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 27.15 | 36.44 | 23.17 | 319.84 | 0.5451 | 745.0 | 688.6 | |
| 0.00 | 1.98 | 0.00 | 1.16 | 26.95 | 36.32 | 23.06 | 319.71 | 0.5420 | 760.0 | 535.0 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 30.58 | 33.03 | 19.77 | 328.10 | 0.5531 | 747.0 | 595.5 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 34.03 | 30.96 | 17.69 | 334.14 | 0.5796 | 666.0 | 547.8 | |
| 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. | |