SDO HMI 2014-10-12 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.84 | 0.00 | 11.68 | 13.82 | 59.12 | 26.66 | 289.54 | 0.4621 | 143.7 | 14.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.70 | 0.00 | 0.42 | 12.08 | 66.74 | 34.28 | 282.58 | 0.5664 | -702.0 | -556.9 | |
| 0.00 | 4.81 | 0.00 | 2.88 | 11.60 | 66.56 | 34.10 | 281.78 | 0.5631 | -734.0 | -528.8 | |
| 0.00 | 1.31 | 0.00 | 0.74 | 12.90 | 59.98 | 27.51 | 286.20 | 0.4709 | 672.0 | 556.1 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 18.50 | 60.61 | 28.15 | 296.95 | 0.5039 | -628.0 | -560.1 | |
| 0.00 | 1.23 | 0.00 | 0.69 | 16.43 | 59.70 | 27.23 | 293.56 | 0.4808 | -348.0 | -362.9 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 15.73 | 59.10 | 26.64 | 292.51 | 0.4691 | -751.0 | -587.8 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 16.14 | 58.82 | 26.35 | 293.53 | 0.4670 | -634.0 | -554.2 | |
| 0.00 | 1.49 | 0.00 | 0.82 | 13.10 | 58.25 | 25.78 | 287.42 | 0.4459 | 736.0 | 613.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 13.34 | 56.18 | 23.71 | 289.11 | 0.4158 | 735.0 | 488.6 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 13.13 | 55.42 | 22.95 | 289.08 | 0.4036 | 487.0 | 434.3 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 12.77 | 55.32 | 22.85 | 288.28 | 0.4006 | 721.0 | 600.4 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 13.40 | 54.84 | 22.38 | 290.10 | 0.3961 | 785.0 | 706.9 | |
| 0.00 | 1.75 | 0.00 | 0.92 | 15.03 | 49.97 | 17.50 | 298.95 | 0.3334 | 670.0 | 597.6 | |
| 0.00 | 1.93 | 0.00 | 1.01 | 14.97 | 49.74 | 17.27 | 299.10 | 0.3297 | 1003.0 | 801.5 | |
| 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. | |