SDO HMI 2014-10-11 07:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.17 | 109.62 | 45.72 | 232.52 | -15.14 | 122.83 | 73.89 | 252.71 | 0.9716 | 208.3 | 41.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 2.11 | -14.03 | 125.01 | 76.07 | 254.23 | 0.9794 | 118.0 | 122.2 | |
| 4.29 | 68.96 | 10.30 | 161.72 | -15.04 | 124.78 | 75.83 | 253.17 | 0.9792 | 197.1 | 73.0 | |
| 3.86 | -2.00 | 8.75 | -2.00 | -14.84 | 124.06 | 75.12 | 253.25 | 0.9766 | 465.0 | 999999 | |
| 1.58 | -2.00 | 3.76 | -2.00 | -15.37 | 124.62 | 75.68 | 252.81 | 0.9789 | 286.8 | 999999 | |
| 3.94 | -2.00 | 8.44 | -2.00 | -14.42 | 123.42 | 74.47 | 253.56 | 0.9740 | 585.8 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.63 | -15.95 | 124.76 | 75.82 | 252.24 | 0.9797 | 186.0 | 181.7 | |
| 0.00 | 0.26 | 0.00 | 0.55 | -14.76 | 123.03 | 74.09 | 253.15 | 0.9727 | 488.0 | 441.0 | |
| 0.00 | 1.14 | 0.00 | 2.35 | -14.90 | 122.82 | 73.87 | 252.97 | 0.9720 | 567.0 | 499.7 | |
| 1.49 | 6.05 | 3.03 | 12.49 | -15.09 | 122.54 | 73.60 | 252.73 | 0.9711 | 511.5 | 422.2 | |
| 0.00 | 1.84 | 0.00 | 3.20 | -14.64 | 120.09 | 71.14 | 252.72 | 0.9601 | -12.0 | -18.8 | |
| 0.00 | 2.63 | 0.00 | 4.45 | -15.05 | 119.44 | 70.50 | 252.18 | 0.9575 | 5.0 | -28.3 | |
| 2.10 | 12.53 | 3.54 | 21.14 | -15.25 | 119.32 | 70.38 | 251.94 | 0.9571 | -332.3 | -117.2 | |
| 0.96 | -12.00 | 1.63 | -12.00 | -15.45 | 119.38 | 70.44 | 251.76 | 0.9576 | -228.3 | 999999 | |
| 0.44 | -12.00 | 0.72 | -12.00 | -15.52 | 118.88 | 69.94 | 251.58 | 0.9553 | -320.0 | 999999 | |
| 0.88 | 3.24 | 1.42 | 5.26 | -17.10 | 118.13 | 69.19 | 249.80 | 0.9533 | -217.0 | -112.3 | |
| 2.63 | 11.83 | 4.13 | 18.62 | -17.10 | 117.52 | 68.58 | 249.67 | 0.9503 | -523.9 | -353.4 | |
| 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. | |