SDO HMI 2014-06-10 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.30 | 0.00 | 12.39 | 6.07 | 256.82 | 24.71 | 284.87 | 0.4255 | 369.0 | 382.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.84 | 8.00 | 273.50 | 41.39 | 281.50 | 0.6704 | -574.0 | -449.4 | |
| 0.00 | 1.00 | 0.00 | 0.65 | 5.24 | 272.72 | 40.62 | 277.50 | 0.6561 | -613.0 | -484.4 | |
| 0.00 | 0.63 | 0.00 | 0.41 | 2.26 | 271.32 | 39.21 | 273.01 | 0.6348 | -502.0 | -445.7 | |
| 0.00 | 0.82 | 0.00 | 0.52 | 4.79 | 271.29 | 39.18 | 277.00 | 0.6366 | -639.0 | -585.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 5.79 | 262.15 | 30.05 | 280.68 | 0.5089 | 754.0 | 580.8 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 6.47 | 261.42 | 29.31 | 282.25 | 0.4998 | 629.0 | 498.2 | |
| 0.00 | 1.72 | 0.00 | 0.97 | 8.81 | 259.05 | 26.94 | 288.07 | 0.4728 | 570.0 | 395.0 | |
| 0.00 | 2.45 | 0.00 | 1.35 | 5.23 | 257.62 | 25.52 | 281.07 | 0.4389 | 650.0 | 521.5 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 4.68 | 256.59 | 24.48 | 280.21 | 0.4214 | 714.0 | 573.8 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 6.92 | 255.96 | 23.85 | 285.75 | 0.4188 | 757.0 | 630.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 6.16 | 254.09 | 21.98 | 285.03 | 0.3869 | 658.0 | 490.2 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 9.17 | 253.76 | 21.65 | 292.65 | 0.3963 | 856.0 | 629.8 | |
| 0.00 | 4.80 | 0.00 | 2.46 | 6.99 | 245.21 | 13.10 | 296.85 | 0.2533 | 829.0 | 627.6 | |
| 0.00 | 2.17 | 0.00 | 1.10 | 1.56 | 243.49 | 11.38 | 275.62 | 0.1991 | 1077.0 | 867.5 | |
| 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. | |