SDO HMI 2014-10-02 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.84 | 282.35 | 125.04 | 615.63 | -10.93 | 245.53 | 75.10 | 257.02 | 0.9715 | 87.2 | 97.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.78 | 165.92 | 63.11 | 432.68 | -10.68 | 248.04 | 77.61 | 257.74 | 0.9830 | 90.5 | 131.4 | |
| 7.22 | -1.00 | 17.78 | -1.00 | -10.89 | 247.23 | 76.80 | 257.39 | 0.9806 | 663.6 | 999999 | |
| 10.66 | 19.55 | 25.43 | 46.55 | -12.98 | 246.42 | 75.99 | 255.16 | 0.9790 | 206.0 | 192.5 | |
| 1.41 | 17.00 | 2.89 | 34.22 | -10.85 | 244.70 | 74.27 | 257.02 | 0.9712 | 447.9 | 398.1 | |
| 0.00 | 2.20 | 0.00 | 5.05 | -13.61 | 245.86 | 75.43 | 254.43 | 0.9775 | -85.0 | -24.5 | |
| 0.00 | 1.85 | 0.00 | 3.43 | -11.83 | 242.97 | 72.54 | 255.71 | 0.9647 | -159.0 | -157.1 | |
| 12.77 | 67.20 | 15.83 | 83.54 | -10.71 | 234.86 | 64.43 | 255.21 | 0.9184 | -613.8 | -166.9 | |
| 0.00 | 0.97 | 0.00 | 1.20 | -11.78 | 234.67 | 64.24 | 254.03 | 0.9187 | -394.0 | -276.0 | |
| 0.00 | 1.94 | 0.00 | 2.32 | -11.16 | 233.85 | 63.42 | 254.49 | 0.9123 | -286.0 | -330.0 | |
| 0.00 | 0.88 | 0.00 | 1.04 | -10.62 | 233.43 | 63.00 | 254.98 | 0.9085 | -432.0 | -410.7 | |
| 0.00 | 1.14 | 0.00 | 1.30 | -9.24 | 232.70 | 62.27 | 256.30 | 0.9010 | 92.0 | 97.5 | |
| 0.00 | 0.97 | 0.00 | 1.13 | -10.78 | 233.22 | 62.79 | 254.75 | 0.9073 | -339.0 | -295.2 | |
| 0.00 | 1.41 | 0.00 | 1.62 | -10.22 | 232.89 | 62.46 | 255.28 | 0.9040 | -509.0 | -410.1 | |
| 0.00 | 1.32 | 0.00 | 1.55 | -11.22 | 233.26 | 62.83 | 254.29 | 0.9083 | -521.0 | -490.7 | |
| 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. | |