SDO HMI 2014-10-08 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.56 | 0.00 | 9.98 | -17.19 | 104.19 | 16.76 | 214.46 | 0.4931 | 93.4 | 94.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.60 | -13.34 | 110.48 | 23.05 | 229.28 | 0.5047 | 811.0 | 636.6 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -13.47 | 110.42 | 22.99 | 229.02 | 0.5053 | 891.0 | 745.2 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -16.48 | 110.43 | 23.00 | 224.65 | 0.5352 | 665.0 | 554.0 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -15.21 | 110.21 | 22.78 | 226.16 | 0.5201 | 790.0 | 602.5 | |
| 0.00 | 1.40 | 0.00 | 0.80 | -14.18 | 109.36 | 21.93 | 226.59 | 0.5005 | 737.0 | 632.5 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -22.78 | 109.25 | 21.82 | 215.57 | 0.5913 | 516.0 | 421.7 | |
| 0.00 | 1.67 | 0.00 | 0.98 | -18.90 | 108.09 | 20.66 | 218.51 | 0.5382 | 724.0 | 547.7 | |
| 0.00 | 2.46 | 0.00 | 1.39 | -15.25 | 107.24 | 19.81 | 222.15 | 0.4893 | 654.0 | 509.6 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -9.24 | 102.71 | 15.28 | 224.53 | 0.3726 | -811.0 | -662.1 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -19.03 | 99.21 | 11.78 | 204.38 | 0.4696 | -660.0 | -528.8 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -19.21 | 98.42 | 10.99 | 202.75 | 0.4673 | -742.0 | -670.1 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -19.03 | 97.89 | 10.46 | 201.92 | 0.4616 | -758.0 | -639.1 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -18.48 | 94.85 | 7.42 | 196.31 | 0.4379 | -745.0 | -507.3 | |
| 0.00 | 1.58 | 0.00 | 0.90 | -22.22 | 93.98 | 6.55 | 192.49 | 0.4907 | -765.0 | -583.3 | |
| 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. | |