SDO HMI 2014-04-24 14:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.75 | 343.86 | 32.98 | 222.97 | 17.92 | 166.28 | 33.66 | 305.28 | 0.6482 | -759.0 | -310.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.75 | 326.51 | 32.98 | 212.10 | 17.92 | 166.43 | 33.81 | 305.15 | 0.6498 | -1252.0 | -359.8 | |
| 0.00 | 2.22 | 0.00 | 1.40 | 17.21 | 164.51 | 31.89 | 305.71 | 0.6237 | 283.0 | 95.2 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 17.05 | 164.44 | 31.82 | 305.54 | 0.6218 | 529.0 | 420.1 | |
| 0.00 | 0.62 | 0.00 | 0.39 | 17.07 | 164.29 | 31.68 | 305.69 | 0.6203 | 588.0 | 581.7 | |
| 0.00 | 3.11 | 0.00 | 1.95 | 17.71 | 163.34 | 30.73 | 307.37 | 0.6147 | 645.0 | 528.4 | |
| 0.00 | 0.98 | 0.00 | 0.61 | 18.17 | 163.32 | 30.70 | 308.00 | 0.6179 | 459.0 | 447.5 | |
| 0.00 | 1.78 | 0.00 | 1.11 | 17.90 | 163.20 | 30.58 | 307.75 | 0.6145 | 801.0 | 693.0 | |
| 0.00 | 0.71 | 0.00 | 0.45 | 18.35 | 163.02 | 30.41 | 308.51 | 0.6162 | 540.0 | 492.8 | |
| 0.00 | 2.67 | 0.00 | 1.67 | 18.08 | 162.82 | 30.21 | 308.32 | 0.6119 | 649.0 | 624.2 | |
| 0.00 | 0.98 | 0.00 | 0.61 | 18.27 | 162.75 | 30.13 | 308.65 | 0.6126 | 636.0 | 521.5 | |
| 0.00 | 1.07 | 0.00 | 0.66 | 17.88 | 162.68 | 30.06 | 308.18 | 0.6087 | 719.0 | 580.2 | |
| 0.00 | 1.16 | 0.00 | 0.72 | 18.53 | 162.69 | 30.07 | 309.05 | 0.6140 | 661.0 | 580.7 | |
| 0.00 | 1.07 | 0.00 | 0.68 | 20.37 | 162.55 | 29.94 | 311.57 | 0.6276 | 642.0 | 489.2 | |
| 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. | |