SDO HMI 2014-08-27 14:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.76 | 313.32 | 82.64 | 355.55 | 7.79 | 344.06 | 64.90 | 275.27 | 0.9026 | -315.9 | -286.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 1.59 | 7.86 | 348.52 | 69.36 | 275.71 | 0.9332 | -160.0 | -153.6 | |
| 0.00 | 0.99 | 0.00 | 1.35 | 8.37 | 348.63 | 69.47 | 276.27 | 0.9336 | 204.0 | 201.9 | |
| 5.65 | 8.70 | 7.54 | 11.63 | 8.40 | 348.12 | 68.96 | 276.25 | 0.9304 | -487.8 | -312.7 | |
| 1.52 | 2.78 | 1.97 | 3.59 | 9.75 | 347.40 | 68.24 | 277.65 | 0.9252 | 202.5 | 252.3 | |
| 0.00 | 1.44 | 0.00 | 1.79 | 7.39 | 346.27 | 67.11 | 275.00 | 0.9188 | 149.0 | 129.7 | |
| 0.00 | 0.90 | 0.00 | 1.11 | 7.62 | 346.11 | 66.95 | 275.24 | 0.9176 | 187.0 | 145.9 | |
| 0.00 | 0.90 | 0.00 | 1.08 | 8.17 | 345.58 | 66.43 | 275.80 | 0.9136 | -456.0 | -465.6 | |
| 18.57 | 291.41 | 21.54 | 328.09 | 7.25 | 344.47 | 65.31 | 274.70 | 0.9061 | 491.4 | -306.2 | |
| 0.99 | -8.00 | 1.11 | -8.00 | 6.66 | 343.51 | 64.35 | 273.96 | 0.8994 | -103.5 | 999999 | |
| 44.22 | -8.00 | 49.62 | -8.00 | 7.94 | 343.58 | 64.42 | 275.39 | 0.8991 | -740.1 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.75 | 6.67 | 341.46 | 62.30 | 273.79 | 0.8832 | 305.0 | 281.8 | |
| 0.81 | 2.42 | 0.86 | 2.58 | 10.52 | 342.20 | 63.04 | 278.19 | 0.8872 | 523.1 | 436.9 | |
| 0.00 | 0.90 | 0.00 | 0.96 | 11.00 | 342.24 | 63.08 | 278.74 | 0.8875 | 373.0 | 279.5 | |
| 0.00 | 0.99 | 0.00 | 1.03 | 9.77 | 341.46 | 62.30 | 277.30 | 0.8816 | -150.0 | -124.4 | |
| 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. | |