SDO HMI 2014-12-09 14:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.85 | 326.94 | 33.19 | 167.24 | -3.86 | 1.26 | 14.02 | 255.14 | 0.2513 | 1046.6 | 384.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.58 | -4.94 | 4.95 | 17.71 | 254.66 | 0.3156 | 896.0 | 800.4 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -5.18 | 4.83 | 17.59 | 253.84 | 0.3147 | 907.0 | 647.5 | |
| 37.50 | 308.28 | 19.21 | 157.70 | -3.99 | 1.51 | 14.27 | 254.86 | 0.2558 | 1318.3 | 395.2 | |
| 1.19 | 9.12 | 0.61 | 4.66 | -2.69 | 1.31 | 14.07 | 259.76 | 0.2478 | 861.2 | 632.8 | |
| 1.19 | -4.00 | 0.61 | -4.00 | -2.37 | 1.21 | 13.97 | 261.00 | 0.2454 | 755.8 | 999999 | |
| 8.01 | -3.00 | 4.10 | -3.00 | -4.11 | 1.17 | 13.93 | 254.06 | 0.2509 | 1372.9 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -2.07 | 1.00 | 13.76 | 262.08 | 0.2410 | -654.0 | -439.3 | |
| 0.00 | 0.51 | 0.00 | 0.26 | -1.45 | 0.78 | 13.54 | 264.58 | 0.2362 | -841.0 | -790.8 | |
| 16.96 | -3.00 | 8.66 | -3.00 | -3.61 | 0.77 | 13.53 | 255.63 | 0.2421 | 1428.9 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -1.60 | 0.63 | 13.39 | 263.89 | 0.2338 | -843.0 | -628.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -2.57 | 359.88 | 12.64 | 259.18 | 0.2235 | 900.0 | 614.3 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -2.78 | 359.10 | 11.85 | 257.53 | 0.2111 | -756.0 | -483.3 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -7.37 | 357.90 | 10.66 | 235.69 | 0.2231 | -814.0 | -753.1 | |
| 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. | |