SDO HMI 2014-09-27 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.82 | 228.55 | 67.16 | 241.22 | 12.42 | 169.20 | -62.82 | 79.55 | 0.8843 | -66.0 | 26.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.44 | 1.85 | 0.42 | 1.75 | 11.34 | 172.98 | -59.05 | 80.89 | 0.8537 | -318.2 | -333.7 | |
| 3.27 | 21.90 | 3.17 | 21.18 | 12.56 | 172.05 | -59.98 | 79.45 | 0.8617 | -725.4 | -426.3 | |
| 0.00 | 1.24 | 0.00 | 1.19 | 12.21 | 172.18 | -59.85 | 79.86 | 0.8606 | -617.0 | -552.4 | |
| 10.51 | 57.50 | 10.33 | 56.68 | 11.87 | 171.62 | -60.41 | 80.24 | 0.8655 | -808.6 | -264.8 | |
| 2.30 | -4.00 | 2.26 | -4.00 | 12.11 | 171.53 | -60.49 | 79.96 | 0.8662 | -625.2 | 999999 | |
| 3.36 | 36.30 | 3.34 | 36.38 | 12.50 | 171.19 | -60.84 | 79.50 | 0.8691 | -490.7 | 95.0 | |
| 6.98 | -4.00 | 6.94 | -4.00 | 11.80 | 171.21 | -60.82 | 80.31 | 0.8690 | -349.8 | 999999 | |
| 4.59 | -6.00 | 4.60 | -6.00 | 12.29 | 170.95 | -61.07 | 79.74 | 0.8711 | -211.3 | 999999 | |
| 1.32 | 3.00 | 1.30 | 2.95 | 10.19 | 171.64 | -60.39 | 82.18 | 0.8658 | -493.7 | -356.3 | |
| 0.00 | 1.06 | 0.00 | 1.05 | 9.77 | 171.39 | -60.64 | 82.65 | 0.8680 | -275.0 | -243.1 | |
| 0.00 | 1.32 | 0.00 | 1.39 | 12.17 | 169.49 | -62.54 | 79.84 | 0.8831 | 97.0 | 77.9 | |
| 1.50 | 52.55 | 1.62 | 56.34 | 13.44 | 168.65 | -63.37 | 78.40 | 0.8895 | 321.5 | 340.3 | |
| 8.92 | -12.00 | 9.69 | -12.00 | 12.94 | 168.33 | -63.70 | 78.95 | 0.8921 | 703.1 | 999999 | |
| 10.33 | 37.18 | 11.63 | 41.82 | 12.59 | 167.35 | -64.68 | 79.31 | 0.8996 | 495.3 | 196.7 | |
| 0.00 | 0.88 | 0.00 | 1.04 | 11.30 | 166.16 | -65.87 | 80.70 | 0.9086 | 366.0 | 331.6 | |
| 3.18 | 6.62 | 4.23 | 8.80 | 13.00 | 162.92 | -69.11 | 78.70 | 0.9299 | -306.7 | -171.7 | |
| 5.12 | 7.15 | 7.63 | 10.65 | 12.12 | 160.50 | -71.53 | 79.53 | 0.9445 | 270.9 | 156.6 | |
| 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. | |