SDO HMI 2014-08-13 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.35 | 391.73 | 34.74 | 221.27 | 15.11 | 133.70 | 27.87 | 289.68 | 0.4811 | -930.5 | -344.3 | |
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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 | 0.68 | 16.92 | 135.61 | 29.78 | 292.26 | 0.5155 | 485.0 | 388.6 | |
| 61.35 | 372.53 | 34.74 | 210.96 | 15.24 | 134.00 | 28.17 | 289.83 | 0.4861 | -1399.4 | -391.0 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 13.72 | 133.01 | 27.18 | 287.18 | 0.4664 | -662.0 | -531.4 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 16.46 | 131.91 | 26.08 | 293.51 | 0.4616 | -700.0 | -518.8 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 18.49 | 129.15 | 23.32 | 299.88 | 0.4348 | -787.0 | -661.0 | |
| 0.00 | 2.71 | 0.00 | 1.45 | 12.65 | 127.17 | 21.34 | 287.79 | 0.3746 | 711.0 | 550.2 | |
| 0.00 | 1.71 | 0.00 | 0.91 | 12.41 | 127.02 | 21.19 | 287.27 | 0.3712 | 982.0 | 783.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 12.16 | 126.40 | 20.57 | 286.99 | 0.3607 | 853.0 | 573.6 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 10.61 | 126.25 | 20.42 | 282.80 | 0.3531 | 809.0 | 600.4 | |
| 0.00 | 1.53 | 0.00 | 0.81 | 9.07 | 125.82 | 19.99 | 278.57 | 0.3428 | 710.0 | 582.2 | |
| 0.00 | 2.62 | 0.00 | 1.38 | 11.60 | 125.99 | 20.16 | 285.70 | 0.3522 | 745.0 | 592.2 | |
| 0.00 | 1.71 | 0.00 | 0.91 | 11.08 | 125.82 | 19.99 | 284.36 | 0.3478 | 835.0 | 660.6 | |
| 0.00 | 2.98 | 0.00 | 1.56 | 10.32 | 124.33 | 18.50 | 282.92 | 0.3216 | 1144.0 | 908.8 | |
| 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. | |