SDO HMI 2014-10-10 18:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.56 | 192.90 | 60.93 | 278.97 | -15.25 | 123.32 | 67.22 | 251.24 | 0.9402 | 166.6 | 92.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.12 | 0.00 | 6.66 | -14.33 | 125.93 | 69.83 | 252.77 | 0.9536 | -271.0 | -251.8 | |
| 1.31 | 131.87 | 2.08 | 201.78 | -14.56 | 125.46 | 69.36 | 252.43 | 0.9515 | 208.7 | 132.4 | |
| 16.29 | -2.00 | 25.42 | -2.00 | -15.18 | 125.01 | 68.92 | 251.71 | 0.9498 | 251.2 | 999999 | |
| 7.36 | -2.00 | 11.01 | -2.00 | -15.06 | 124.16 | 68.06 | 251.65 | 0.9452 | 595.0 | 999999 | |
| 3.94 | -2.00 | 5.69 | -2.00 | -14.51 | 123.47 | 67.38 | 252.06 | 0.9408 | 752.1 | 999999 | |
| 0.00 | 2.19 | 0.00 | 2.97 | -15.05 | 121.91 | 65.81 | 251.15 | 0.9324 | 676.0 | 552.3 | |
| 1.40 | 13.48 | 1.80 | 17.44 | -15.56 | 120.43 | 64.33 | 250.25 | 0.9242 | -70.5 | 236.7 | |
| 0.88 | -7.00 | 1.12 | -7.00 | -15.84 | 120.30 | 64.20 | 249.93 | 0.9238 | -236.8 | 999999 | |
| 4.55 | 17.69 | 5.65 | 21.92 | -15.35 | 119.59 | 63.50 | 250.26 | 0.9185 | -296.5 | -37.3 | |
| 2.54 | 12.78 | 3.07 | 15.54 | -16.65 | 118.60 | 62.50 | 248.63 | 0.9143 | -516.4 | -49.7 | |
| 0.00 | 0.79 | 0.00 | 0.91 | -15.40 | 117.52 | 61.42 | 249.67 | 0.9047 | -354.0 | -339.1 | |
| 4.29 | 8.32 | 5.09 | 9.86 | -16.91 | 117.93 | 61.84 | 248.17 | 0.9104 | -527.1 | -366.5 | |
| 0.00 | 1.66 | 0.00 | 1.89 | -16.04 | 116.94 | 60.84 | 248.82 | 0.9019 | -546.0 | -401.6 | |
| 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. | |