SDO HMI 2014-04-08 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 32.24 | 0.00 | 16.76 | -9.84 | 8.74 | 17.17 | 256.00 | 0.3041 | 262.4 | 422.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.50 | 0.00 | 0.79 | -10.23 | 12.02 | 20.44 | 257.23 | 0.3540 | -730.0 | -449.0 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -8.18 | 11.32 | 19.74 | 262.88 | 0.3384 | 823.0 | 673.2 | |
| 0.00 | 6.78 | 0.00 | 3.56 | -8.58 | 11.01 | 19.44 | 261.60 | 0.3341 | 762.0 | 695.3 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -8.88 | 11.03 | 19.46 | 260.71 | 0.3349 | 622.0 | 477.2 | |
| 0.00 | 2.64 | 0.00 | 1.38 | -9.14 | 10.53 | 18.96 | 259.75 | 0.3273 | 508.0 | 717.0 | |
| 0.00 | 2.20 | 0.00 | 1.15 | -8.82 | 10.41 | 18.84 | 260.71 | 0.3248 | 808.0 | 660.6 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -10.21 | 9.02 | 17.44 | 255.60 | 0.3059 | 638.0 | 505.1 | |
| 0.00 | 2.64 | 0.00 | 1.37 | -10.52 | 8.84 | 17.27 | 254.49 | 0.3042 | 732.0 | 575.5 | |
| 0.00 | 5.11 | 0.00 | 2.65 | -10.10 | 8.72 | 17.15 | 255.76 | 0.3008 | 692.0 | 696.3 | |
| 0.00 | 1.76 | 0.00 | 0.90 | -7.41 | 6.05 | 14.48 | 264.14 | 0.2504 | -915.0 | -719.0 | |
| 0.00 | 1.59 | 0.00 | 0.81 | -7.66 | 5.65 | 14.08 | 263.00 | 0.2440 | -871.0 | -659.9 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -8.07 | 5.01 | 13.44 | 261.01 | 0.2340 | -718.0 | -594.9 | |
| 0.00 | 0.62 | 0.00 | 0.32 | -15.57 | 2.96 | 11.38 | 228.93 | 0.2534 | 537.0 | 435.7 | |
| 0.00 | 2.99 | 0.00 | 1.53 | -15.81 | 2.94 | 11.37 | 228.15 | 0.2557 | 786.0 | 696.6 | |
| 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. | |