SDO HMI 2014-04-15 10:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.59 | 383.30 | 32.19 | 214.06 | 11.92 | 274.96 | 21.28 | 309.72 | 0.4636 | -798.3 | -360.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.79 | 359.95 | 31.76 | 201.31 | 11.82 | 275.30 | 21.62 | 309.03 | 0.4662 | -1429.6 | -425.7 | |
| 0.00 | 1.06 | 0.00 | 0.59 | 14.58 | 272.32 | 18.64 | 317.68 | 0.4613 | -636.0 | -560.4 | |
| 0.00 | 0.35 | 0.00 | 0.19 | 12.97 | 270.72 | 17.04 | 317.71 | 0.4262 | 548.0 | 587.2 | |
| 0.00 | 1.33 | 0.00 | 0.72 | 11.29 | 270.61 | 16.93 | 315.06 | 0.4059 | -561.0 | -483.5 | |
| 0.00 | 2.30 | 0.00 | 1.26 | 12.81 | 270.65 | 16.96 | 317.58 | 0.4235 | 707.0 | 675.6 | |
| 0.00 | 2.48 | 0.00 | 1.35 | 12.93 | 270.46 | 16.78 | 318.08 | 0.4230 | 906.0 | 776.9 | |
| 0.00 | 1.68 | 0.00 | 0.92 | 13.37 | 270.43 | 16.75 | 318.85 | 0.4278 | 604.0 | 432.4 | |
| 0.80 | 2.48 | 0.43 | 1.35 | 13.08 | 270.12 | 16.44 | 318.91 | 0.4211 | 1017.4 | 829.3 | |
| 0.00 | 1.59 | 0.00 | 0.87 | 13.27 | 270.10 | 16.42 | 319.25 | 0.4232 | 642.0 | 558.9 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 14.29 | 269.17 | 15.49 | 322.44 | 0.4264 | 725.0 | 573.0 | |
| 0.00 | 1.50 | 0.00 | 0.82 | 14.35 | 268.98 | 15.30 | 322.86 | 0.4253 | 903.0 | 732.9 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 14.41 | 268.76 | 15.08 | 323.35 | 0.4239 | 749.0 | 629.6 | |
| 0.00 | 3.45 | 0.00 | 1.89 | 14.82 | 268.53 | 14.85 | 324.35 | 0.4270 | 676.0 | 567.9 | |
| 0.00 | 1.68 | 0.00 | 0.92 | 14.53 | 268.26 | 14.58 | 324.44 | 0.4207 | 941.0 | 857.2 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 11.90 | 266.04 | 12.36 | 324.93 | 0.3660 | 871.0 | 576.1 | |
| 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. | |