SDO HMI 2014-12-09 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.95 | 348.09 | 30.28 | 175.85 | -3.84 | 1.27 | 10.75 | 250.99 | 0.1978 | 1147.2 | 403.5 | |
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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 | 0.57 | -4.99 | 4.91 | 14.38 | 251.22 | 0.2626 | 953.0 | 768.5 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -5.22 | 4.79 | 14.27 | 250.22 | 0.2620 | 967.0 | 789.6 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -4.81 | 4.75 | 14.23 | 251.69 | 0.2591 | 884.0 | 689.2 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -4.01 | 4.43 | 13.91 | 254.36 | 0.2501 | 807.0 | 618.1 | |
| 33.60 | 328.82 | 16.99 | 166.10 | -3.98 | 1.52 | 11.00 | 250.73 | 0.2025 | 1390.8 | 405.2 | |
| 8.10 | -5.00 | 4.09 | -5.00 | -4.04 | 1.16 | 10.64 | 249.85 | 0.1970 | 1451.9 | 999999 | |
| 0.00 | 4.78 | 0.00 | 2.41 | -2.47 | 1.08 | 10.56 | 257.60 | 0.1884 | 833.0 | 674.4 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -1.70 | 1.08 | 10.56 | 261.66 | 0.1859 | -453.0 | -305.5 | |
| 0.68 | 3.41 | 0.34 | 1.72 | -1.70 | 0.81 | 10.29 | 261.45 | 0.1813 | -970.0 | -689.8 | |
| 17.57 | -5.00 | 8.86 | -5.00 | -3.59 | 0.76 | 10.24 | 251.37 | 0.1881 | 1479.9 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.64 | -2.38 | 0.75 | 10.23 | 257.70 | 0.1825 | 1020.0 | 819.1 | |
| 0.00 | 0.94 | 0.00 | 0.47 | -1.97 | 0.63 | 10.11 | 259.82 | 0.1790 | -767.0 | -589.2 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -5.40 | 359.55 | 9.03 | 239.72 | 0.1818 | 969.0 | 765.7 | |
| 0.00 | 1.28 | 0.00 | 0.64 | -5.46 | 359.25 | 8.73 | 238.60 | 0.1779 | 762.0 | 536.7 | |
| 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. | |