SDO HMI 2014-09-15 18:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.46 | 24.78 | 2.41 | 17.28 | -15.33 | 65.02 | 39.00 | 239.59 | 0.7059 | 315.2 | 404.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.65 | -17.03 | 67.51 | 41.49 | 239.02 | 0.7411 | 611.0 | 500.7 | |
| 0.00 | 1.78 | 0.00 | 1.27 | -15.19 | 66.59 | 40.57 | 240.73 | 0.7218 | 569.0 | 466.3 | |
| 0.00 | 0.98 | 0.00 | 0.69 | -15.08 | 66.35 | 40.34 | 240.73 | 0.7188 | 618.0 | 587.6 | |
| 0.00 | 4.62 | 0.00 | 3.26 | -15.11 | 66.03 | 40.02 | 240.49 | 0.7156 | 816.0 | 693.6 | |
| 2.22 | 4.88 | 1.56 | 3.43 | -15.80 | 65.34 | 39.32 | 239.20 | 0.7121 | 689.5 | 597.0 | |
| 0.00 | 0.98 | 0.00 | 0.68 | -15.09 | 65.01 | 39.00 | 239.89 | 0.7046 | 568.0 | 494.9 | |
| 0.00 | 2.31 | 0.00 | 1.60 | -14.73 | 64.94 | 38.92 | 240.30 | 0.7018 | 786.0 | 623.3 | |
| 0.00 | 0.62 | 0.00 | 0.43 | -14.96 | 64.94 | 38.93 | 240.02 | 0.7031 | 671.0 | 645.7 | |
| 0.00 | 1.51 | 0.00 | 1.05 | -15.54 | 64.95 | 38.93 | 239.29 | 0.7066 | 783.0 | 664.4 | |
| 0.00 | 1.15 | 0.00 | 0.80 | -16.10 | 63.92 | 37.90 | 237.90 | 0.6990 | -633.0 | -477.3 | |
| 0.00 | 1.42 | 0.00 | 0.99 | -16.73 | 63.94 | 37.92 | 237.14 | 0.7030 | -572.0 | -515.2 | |
| 1.24 | 2.04 | 0.85 | 1.40 | -15.86 | 63.31 | 37.29 | 237.80 | 0.6910 | -710.8 | -575.4 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -15.91 | 63.16 | 37.14 | 237.63 | 0.6898 | -800.0 | -710.3 | |
| 0.00 | 1.33 | 0.00 | 0.85 | -11.30 | 60.32 | 34.31 | 241.84 | 0.6292 | 654.0 | 393.3 | |
| 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. | |