SDO HMI 2014-10-13 17:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.24 | 0.00 | 11.41 | 15.16 | 357.28 | -19.79 | 61.64 | 0.3656 | -479.7 | -451.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.62 | 0.00 | 1.35 | 14.55 | 3.43 | -13.64 | 56.37 | 0.2754 | -855.0 | -676.2 | |
| 0.00 | 2.80 | 0.00 | 1.44 | 14.42 | 3.09 | -13.98 | 57.39 | 0.2791 | -861.0 | -737.8 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 14.11 | 2.73 | -14.34 | 58.97 | 0.2817 | -826.0 | -658.7 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 14.00 | 2.13 | -14.94 | 60.25 | 0.2895 | -791.0 | -690.5 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 14.62 | 0.09 | -16.98 | 61.33 | 0.3235 | -880.0 | -704.2 | |
| 0.00 | 0.35 | 0.00 | 0.18 | 13.95 | 359.98 | -17.09 | 63.36 | 0.3204 | -402.0 | -567.0 | |
| 0.00 | 2.97 | 0.00 | 1.56 | 14.55 | 359.91 | -17.17 | 61.76 | 0.3257 | -1031.0 | -822.9 | |
| 0.00 | 2.80 | 0.00 | 1.47 | 14.91 | 359.75 | -17.32 | 60.97 | 0.3306 | -882.0 | -748.8 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 14.98 | 359.03 | -18.04 | 61.67 | 0.3414 | -819.0 | -540.0 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 15.03 | 358.79 | -18.28 | 61.81 | 0.3452 | -673.0 | -572.9 | |
| 0.00 | 0.61 | 0.00 | 0.33 | 16.27 | 355.09 | -21.98 | 62.64 | 0.4062 | -625.0 | -470.3 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 17.49 | 344.80 | -32.27 | 67.12 | 0.5548 | 691.0 | 538.2 | |
| 0.00 | 1.22 | 0.00 | 0.75 | 17.03 | 341.96 | -35.11 | 69.12 | 0.5908 | 654.0 | 579.0 | |
| 0.00 | 1.40 | 0.00 | 0.86 | 17.21 | 341.84 | -35.23 | 68.88 | 0.5929 | 584.0 | 507.2 | |
| 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. | |