SDO HMI 2014-09-13 15:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.72 | 104.22 | 13.59 | 57.29 | -15.78 | 65.82 | 11.74 | 206.74 | 0.4373 | 661.1 | 480.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.07 | 0.00 | 0.59 | -16.35 | 67.46 | 13.38 | 209.25 | 0.4563 | 670.0 | 476.3 | |
| 3.73 | 90.70 | 2.06 | 49.84 | -15.87 | 66.91 | 12.83 | 208.77 | 0.4457 | 787.7 | 566.5 | |
| 0.00 | 3.11 | 0.00 | 1.73 | -16.36 | 66.72 | 12.64 | 207.87 | 0.4509 | 797.0 | 617.4 | |
| 1.60 | -2.00 | 0.88 | -2.00 | -15.86 | 66.53 | 12.45 | 208.05 | 0.4427 | 932.4 | 999999 | |
| 5.69 | -2.00 | 3.13 | -2.00 | -15.72 | 66.23 | 12.15 | 207.63 | 0.4386 | 965.2 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -16.51 | 66.25 | 12.17 | 206.82 | 0.4496 | 570.0 | 462.8 | |
| 5.07 | -2.00 | 2.79 | -2.00 | -15.58 | 66.03 | 11.95 | 207.39 | 0.4353 | 1088.7 | 999999 | |
| 8.63 | -2.00 | 4.73 | -2.00 | -15.45 | 65.80 | 11.72 | 207.09 | 0.4317 | 1184.9 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.69 | -15.97 | 65.73 | 11.65 | 206.40 | 0.4385 | 624.0 | 493.6 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -16.34 | 64.79 | 10.71 | 204.17 | 0.4375 | 800.0 | 593.3 | |
| 0.00 | 1.69 | 0.00 | 0.93 | -17.72 | 61.85 | 7.77 | 197.03 | 0.4417 | -673.0 | -515.4 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -17.06 | 61.79 | 7.71 | 197.38 | 0.4314 | -757.0 | -595.4 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -18.79 | 59.62 | 5.54 | 191.80 | 0.4492 | -576.0 | -501.1 | |
| 0.00 | 2.76 | 0.00 | 1.50 | -16.75 | 58.74 | 4.66 | 190.86 | 0.4149 | -627.0 | -587.4 | |
| 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. | |