SDO HMI 2014-10-07 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.69 | 157.46 | 43.90 | 178.05 | -12.30 | 165.80 | 61.35 | 252.87 | 0.8983 | 234.4 | 65.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.90 | 128.65 | 24.44 | 150.55 | -12.49 | 166.97 | 62.52 | 252.98 | 0.9077 | 556.4 | 115.1 | |
| 7.99 | -1.00 | 9.10 | -1.00 | -12.01 | 166.31 | 61.86 | 253.32 | 0.9022 | 698.1 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.88 | -11.55 | 165.74 | 61.29 | 253.68 | 0.8972 | 289.0 | 392.6 | |
| 0.61 | -1.00 | 0.69 | -1.00 | -12.05 | 165.74 | 61.29 | 253.14 | 0.8981 | 544.6 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.87 | -12.04 | 165.35 | 60.90 | 253.05 | 0.8952 | 633.0 | 578.2 | |
| 0.00 | 1.05 | 0.00 | 1.11 | -13.80 | 163.52 | 59.06 | 250.63 | 0.8849 | -364.0 | -290.6 | |
| 0.00 | 2.11 | 0.00 | 2.11 | -11.70 | 162.26 | 57.81 | 252.59 | 0.8705 | 209.0 | 229.7 | |
| 6.94 | 11.68 | 6.62 | 11.15 | -11.57 | 160.64 | 56.18 | 252.26 | 0.8566 | -625.8 | -371.1 | |
| 0.00 | 0.97 | 0.00 | 0.92 | -11.92 | 160.30 | 55.85 | 251.78 | 0.8545 | -449.0 | -360.5 | |
| 3.25 | 4.92 | 3.05 | 4.62 | -11.94 | 159.93 | 55.47 | 251.63 | 0.8514 | -641.1 | -491.4 | |
| 0.00 | 0.97 | 0.00 | 0.88 | -12.34 | 158.50 | 54.04 | 250.73 | 0.8398 | -501.0 | -386.5 | |
| 0.00 | 3.25 | 0.00 | 2.91 | -12.41 | 157.89 | 53.44 | 250.45 | 0.8346 | -624.0 | -522.8 | |
| 0.00 | 1.23 | 0.00 | 1.10 | -12.80 | 157.70 | 53.24 | 249.93 | 0.8339 | -432.0 | -464.1 | |
| 0.00 | 1.05 | 0.00 | 0.95 | -13.25 | 157.79 | 53.33 | 249.45 | 0.8360 | -589.0 | -537.6 | |
| 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. | |