SDO HMI 2014-09-12 21:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.40 | 158.77 | 19.08 | 85.57 | -15.86 | 66.03 | 2.06 | 185.08 | 0.3963 | 676.8 | 396.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.53 | 146.13 | 0.29 | 78.72 | -16.08 | 67.07 | 3.10 | 187.49 | 0.4008 | 820.7 | 477.4 | |
| 0.89 | -1.00 | 0.48 | -1.00 | -15.95 | 66.98 | 3.01 | 187.30 | 0.3985 | 1039.8 | 999999 | |
| 0.00 | 2.85 | 0.00 | 1.54 | -16.44 | 66.92 | 2.95 | 187.01 | 0.4062 | 506.0 | 409.2 | |
| 25.26 | -1.00 | 13.62 | -1.00 | -15.84 | 66.41 | 2.44 | 185.97 | 0.3958 | 1161.5 | 999999 | |
| 6.85 | -1.00 | 3.68 | -1.00 | -15.55 | 66.09 | 2.12 | 185.27 | 0.3905 | 1353.9 | 999999 | |
| 1.87 | -1.00 | 1.01 | -1.00 | -15.68 | 65.87 | 1.91 | 184.70 | 0.3923 | 1061.9 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.57 | -14.92 | 63.96 | -0.00 | 179.99 | 0.3788 | 846.0 | 632.4 | |
| 0.00 | 1.51 | 0.00 | 0.82 | -17.09 | 62.13 | -1.84 | 175.74 | 0.4148 | -913.0 | -702.5 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -17.02 | 61.85 | -2.12 | 175.08 | 0.4141 | -800.0 | -673.4 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -17.12 | 61.75 | -2.22 | 174.88 | 0.4158 | -544.0 | -551.7 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -18.67 | 59.91 | -4.06 | 171.28 | 0.4436 | -953.0 | -835.5 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -19.00 | 59.78 | -4.19 | 171.11 | 0.4491 | -653.0 | -546.4 | |
| 0.00 | 1.25 | 0.00 | 0.66 | -13.83 | 59.86 | -4.11 | 169.04 | 0.3674 | -918.0 | -732.1 | |
| 0.00 | 2.13 | 0.00 | 1.16 | -16.23 | 57.92 | -6.05 | 165.72 | 0.4120 | -684.0 | -574.7 | |
| 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. | |