SDO HMI 2014-04-10 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.79 | 36.24 | 14.92 | 41.18 | -8.31 | 26.46 | 64.58 | 263.60 | 0.8999 | 261.3 | 289.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.68 | 6.35 | 2.01 | 7.66 | -7.20 | 28.03 | 66.15 | 264.78 | 0.9129 | 567.0 | 435.1 | |
| 1.85 | 7.06 | 2.17 | 8.28 | -7.65 | 27.42 | 65.54 | 264.32 | 0.9083 | 637.6 | 515.2 | |
| 2.21 | 5.73 | 2.60 | 6.75 | -8.64 | 27.58 | 65.70 | 263.23 | 0.9091 | 477.2 | 407.8 | |
| 0.79 | -2.00 | 0.93 | -2.00 | -7.84 | 27.32 | 65.44 | 264.12 | 0.9076 | 596.4 | 999999 | |
| 0.97 | 2.73 | 1.14 | 3.20 | -9.14 | 27.45 | 65.57 | 262.68 | 0.9081 | 455.6 | 350.7 | |
| 4.23 | 6.79 | 4.89 | 7.84 | -8.39 | 26.98 | 65.10 | 263.53 | 0.9049 | 556.8 | 440.0 | |
| 0.53 | 2.03 | 0.60 | 2.31 | -7.19 | 26.56 | 64.68 | 264.89 | 0.9022 | -192.5 | -126.9 | |
| 0.53 | 1.50 | 0.58 | 1.64 | -8.32 | 25.47 | 63.59 | 263.68 | 0.8935 | -157.5 | -102.2 | |
| 0.00 | 0.62 | 0.00 | 0.65 | -10.52 | 24.42 | 62.54 | 261.25 | 0.8846 | 358.0 | 379.0 | |
| 0.00 | 0.26 | 0.00 | 0.24 | -10.85 | 18.89 | 57.01 | 260.93 | 0.8364 | -419.0 | -376.0 | |
| 0.00 | 1.32 | 0.00 | 1.12 | -13.26 | 16.46 | 54.58 | 257.95 | 0.8132 | -497.0 | -377.4 | |
| 0.00 | 0.35 | 0.00 | 0.29 | -10.24 | 14.61 | 52.73 | 261.67 | 0.7938 | -201.0 | -249.5 | |
| 0.00 | 0.79 | 0.00 | 0.64 | -10.32 | 14.28 | 52.40 | 261.56 | 0.7903 | -609.0 | -473.0 | |
| 0.00 | 0.71 | 0.00 | 0.56 | -10.62 | 13.25 | 51.37 | 261.16 | 0.7794 | -520.0 | -475.5 | |
| 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. | |