SDO HMI 2014-09-06 12:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.53 | 83.03 | 22.18 | 44.45 | -14.99 | 148.62 | 0.45 | 181.17 | 0.3799 | 131.8 | -203.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.88 | 0.00 | 1.01 | -16.17 | 149.04 | 0.87 | 182.10 | 0.3992 | -700.0 | -664.1 | |
| 13.48 | 36.07 | 7.14 | 19.11 | -13.40 | 149.00 | 0.83 | 182.29 | 0.3542 | 1038.8 | 651.7 | |
| 9.02 | 13.93 | 4.88 | 7.54 | -16.57 | 149.01 | 0.84 | 182.00 | 0.4055 | -983.2 | -746.9 | |
| 4.29 | -2.00 | 2.27 | -2.00 | -13.24 | 148.78 | 0.61 | 181.71 | 0.3514 | 1145.2 | 999999 | |
| 6.16 | -2.00 | 3.27 | -2.00 | -13.63 | 148.66 | 0.49 | 181.34 | 0.3577 | 971.7 | 999999 | |
| 1.34 | -2.00 | 0.71 | -2.00 | -13.88 | 148.66 | 0.49 | 181.32 | 0.3619 | 813.5 | 999999 | |
| 1.96 | 20.18 | 1.06 | 10.92 | -16.50 | 148.57 | 0.40 | 180.95 | 0.4043 | -1070.8 | -806.2 | |
| 0.00 | 1.16 | 0.00 | 0.62 | -14.27 | 148.50 | 0.33 | 180.89 | 0.3682 | 728.0 | 521.5 | |
| 1.88 | -7.00 | 1.02 | -7.00 | -16.63 | 148.41 | 0.24 | 180.57 | 0.4063 | -847.2 | 999999 | |
| 3.04 | -7.00 | 1.64 | -7.00 | -16.40 | 148.28 | 0.12 | 180.28 | 0.4026 | -1173.2 | 999999 | |
| 0.00 | 1.96 | 0.00 | 1.04 | -13.88 | 147.94 | -0.23 | 179.39 | 0.3618 | 598.0 | 447.0 | |
| 0.00 | 1.52 | 0.00 | 0.82 | -16.53 | 147.91 | -0.26 | 179.37 | 0.4047 | -753.0 | -607.4 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -16.20 | 147.47 | -0.70 | 178.30 | 0.3996 | -696.0 | -500.9 | |
| 0.00 | 1.07 | 0.00 | 0.57 | -14.27 | 147.47 | -0.69 | 178.17 | 0.3684 | 630.0 | 447.7 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -15.74 | 147.37 | -0.79 | 178.04 | 0.3922 | -648.0 | -600.6 | |
| 0.00 | 2.05 | 0.00 | 1.09 | -14.44 | 147.38 | -0.79 | 177.93 | 0.3711 | 866.0 | 535.8 | |
| 0.36 | 1.34 | 0.19 | 0.72 | -15.32 | 147.22 | -0.95 | 177.61 | 0.3854 | -812.5 | -735.3 | |
| 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. | |