SDO HMI 2014-01-13 00:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.19 | 63.54 | 39.61 | 106.57 | 8.43 | 103.19 | 71.75 | 280.31 | 0.9531 | 209.0 | 69.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.99 | 9.60 | 11.34 | 27.39 | 6.84 | 110.67 | 79.23 | 277.76 | 0.9852 | 20.5 | -63.3 | |
| 2.04 | 3.14 | 3.99 | 6.13 | 6.69 | 106.15 | 74.70 | 278.07 | 0.9687 | -229.1 | -219.0 | |
| 0.00 | 0.76 | 0.00 | 1.49 | 6.98 | 106.05 | 74.61 | 278.39 | 0.9685 | -322.0 | -296.3 | |
| 0.51 | 1.36 | 0.89 | 2.36 | 6.54 | 104.15 | 72.70 | 278.15 | 0.9595 | -237.0 | -191.7 | |
| 0.00 | 0.76 | 0.00 | 1.10 | 7.77 | 100.38 | 68.93 | 279.92 | 0.9402 | 201.0 | 149.6 | |
| 0.00 | 1.27 | 0.00 | 1.82 | 7.88 | 100.25 | 68.81 | 280.05 | 0.9395 | 223.0 | 210.7 | |
| 0.00 | 2.04 | 0.00 | 3.04 | 9.46 | 100.90 | 69.46 | 281.63 | 0.9445 | -326.0 | -261.1 | |
| 2.38 | 37.56 | 3.47 | 53.63 | 9.49 | 100.48 | 69.04 | 281.72 | 0.9422 | 105.4 | 181.3 | |
| 3.40 | -8.00 | 4.87 | -8.00 | 9.29 | 100.14 | 68.70 | 281.55 | 0.9400 | 378.1 | 999999 | |
| 0.00 | 1.02 | 0.00 | 1.50 | 10.10 | 100.51 | 69.07 | 282.35 | 0.9428 | -173.0 | -145.1 | |
| 6.88 | -8.00 | 9.68 | -8.00 | 9.37 | 99.68 | 68.24 | 281.72 | 0.9374 | 604.1 | 999999 | |
| 3.99 | 5.61 | 5.37 | 7.55 | 9.30 | 98.70 | 67.25 | 281.79 | 0.9313 | 454.3 | 341.6 | |
| 0.00 | 0.42 | 0.00 | 0.56 | 9.08 | 98.15 | 66.70 | 281.65 | 0.9277 | 330.0 | 252.6 | |
| 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. | |