SDO HMI 2014-03-10 10:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.35 | 54.27 | 5.80 | 27.69 | 6.18 | 11.29 | 2.77 | 348.44 | 0.2401 | 25.2 | 168.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.56 | 0.00 | 0.80 | 4.12 | 18.31 | 9.79 | 318.96 | 0.2596 | 870.0 | 593.8 | |
| 2.51 | 4.51 | 1.28 | 2.30 | 5.91 | 13.99 | 5.47 | 337.29 | 0.2469 | -1111.6 | -793.2 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 5.85 | 13.72 | 5.20 | 338.21 | 0.2441 | -701.0 | -620.5 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 6.21 | 13.63 | 5.12 | 339.08 | 0.2494 | -1042.0 | -812.2 | |
| 0.69 | 4.34 | 0.36 | 2.22 | 6.73 | 13.16 | 4.64 | 341.54 | 0.2550 | -1107.9 | -864.9 | |
| 0.43 | 2.08 | 0.22 | 1.06 | 5.93 | 13.03 | 4.51 | 340.99 | 0.2414 | -958.8 | -771.5 | |
| 2.34 | 5.12 | 1.20 | 2.62 | 7.33 | 11.48 | 2.96 | 348.46 | 0.2575 | -1022.1 | -713.1 | |
| 0.78 | 5.55 | 0.40 | 2.82 | 5.19 | 10.75 | 2.23 | 349.77 | 0.2193 | 1119.4 | 783.2 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 5.58 | 10.36 | 1.84 | 351.78 | 0.2249 | 1033.0 | 885.0 | |
| 0.00 | 2.77 | 0.00 | 1.42 | 7.45 | 10.37 | 1.85 | 352.78 | 0.2565 | 400.0 | 316.2 | |
| 0.61 | 1.99 | 0.31 | 1.02 | 7.54 | 10.13 | 1.61 | 353.75 | 0.2575 | -884.4 | -683.9 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 6.87 | 9.95 | 1.43 | 354.19 | 0.2458 | 914.0 | 684.6 | |
| 3.99 | 16.47 | 2.03 | 8.38 | 5.88 | 9.85 | 1.34 | 354.16 | 0.2290 | 1088.8 | 603.5 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 6.96 | 9.74 | 1.22 | 355.07 | 0.2470 | 801.0 | 666.3 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 6.19 | 8.72 | 0.20 | 359.14 | 0.2331 | 880.0 | 783.8 | |
| 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. | |