SDO HMI 2014-04-24 17:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.04 | 74.73 | 15.78 | 66.97 | -10.34 | 187.58 | 56.62 | 260.74 | 0.8338 | 61.4 | 157.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.49 | 40.70 | 2.32 | 37.94 | -10.09 | 189.15 | 58.19 | 261.09 | 0.8489 | 703.0 | 265.6 | |
| 2.04 | -1.00 | 1.89 | -1.00 | -10.11 | 188.87 | 57.90 | 261.07 | 0.8463 | 770.4 | 999999 | |
| 1.42 | 9.51 | 1.31 | 8.70 | -9.55 | 188.60 | 57.63 | 261.73 | 0.8438 | 762.1 | 502.5 | |
| 3.11 | -3.00 | 2.85 | -3.00 | -9.67 | 188.63 | 57.67 | 261.59 | 0.8441 | 807.3 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.96 | -10.91 | 187.89 | 56.93 | 260.09 | 0.8374 | 425.0 | 446.7 | |
| 0.00 | 1.24 | 0.00 | 1.13 | -13.09 | 188.27 | 57.30 | 257.50 | 0.8417 | 236.0 | 295.3 | |
| 0.00 | 0.44 | 0.00 | 0.38 | -11.12 | 185.59 | 54.63 | 259.75 | 0.8153 | -310.0 | -336.0 | |
| 0.00 | 0.98 | 0.00 | 0.82 | -9.36 | 185.09 | 54.13 | 261.91 | 0.8098 | -246.0 | -262.1 | |
| 1.07 | 2.75 | 0.90 | 2.32 | -10.88 | 185.10 | 54.14 | 260.02 | 0.8103 | -440.2 | -422.6 | |
| 0.00 | 0.89 | 0.00 | 0.74 | -11.12 | 184.79 | 53.83 | 259.72 | 0.8073 | -165.0 | -295.5 | |
| 6.58 | 8.97 | 5.44 | 7.42 | -10.84 | 184.36 | 53.39 | 260.05 | 0.8027 | -689.7 | -422.4 | |
| 0.00 | 1.87 | 0.00 | 1.50 | -10.74 | 183.01 | 52.04 | 260.10 | 0.7886 | -641.0 | -506.1 | |
| 0.00 | 3.73 | 0.00 | 2.99 | -11.14 | 182.96 | 51.99 | 259.59 | 0.7883 | -602.0 | -549.6 | |
| 1.33 | 2.58 | 1.07 | 2.07 | -12.21 | 182.99 | 52.02 | 258.23 | 0.7892 | 433.3 | 440.6 | |
| 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. | |