SDO HMI 2014-10-13 15:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.25 | 315.46 | 54.00 | 323.41 | -8.97 | 318.87 | -59.30 | 103.79 | 0.8741 | 504.5 | 184.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.76 | 269.48 | 18.89 | 259.12 | -8.58 | 321.05 | -57.12 | 103.82 | 0.8573 | 851.9 | 208.7 | |
| 27.19 | -1.00 | 26.21 | -1.00 | -9.12 | 320.86 | -57.31 | 104.39 | 0.8600 | 689.4 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.90 | -9.75 | 318.64 | -59.53 | 104.55 | 0.8796 | 258.0 | 220.6 | |
| 0.00 | 1.66 | 0.00 | 1.71 | -9.16 | 318.69 | -59.48 | 103.90 | 0.8781 | 276.0 | 216.7 | |
| 0.00 | 1.31 | 0.00 | 1.57 | -8.55 | 314.02 | -64.15 | 102.22 | 0.9124 | -542.0 | -472.1 | |
| 0.00 | 0.96 | 0.00 | 1.15 | -8.20 | 314.13 | -64.05 | 101.87 | 0.9111 | -317.0 | -297.3 | |
| 0.00 | 0.52 | 0.00 | 0.67 | -9.29 | 312.69 | -65.49 | 102.75 | 0.9223 | -339.0 | -377.0 | |
| 0.00 | 0.52 | 0.00 | 0.72 | -8.95 | 310.82 | -67.35 | 102.03 | 0.9337 | -290.0 | -354.5 | |
| 0.35 | 16.79 | 0.50 | 24.37 | -9.89 | 310.03 | -68.14 | 102.88 | 0.9394 | -283.0 | 149.3 | |
| 5.25 | 19.67 | 7.39 | 27.82 | -8.92 | 310.19 | -67.98 | 101.89 | 0.9375 | -314.8 | 26.8 | |
| 0.70 | -9.00 | 1.01 | -9.00 | -9.75 | 309.84 | -68.33 | 102.70 | 0.9404 | -268.5 | 999999 | |
| 0.00 | 0.79 | 0.00 | 1.14 | -9.07 | 309.55 | -68.63 | 101.93 | 0.9414 | 354.0 | 338.7 | |
| 0.00 | 2.89 | 0.00 | 4.24 | -9.32 | 309.27 | -68.90 | 102.14 | 0.9432 | 455.0 | 405.7 | |
| 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. | |