SDO HMI 2014-11-04 15:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.78 | 38.44 | 6.53 | 20.03 | 5.57 | 70.42 | -17.61 | 83.86 | 0.3034 | -189.6 | 142.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.23 | 18.49 | 2.16 | 9.44 | 5.83 | 74.10 | -13.93 | 82.05 | 0.2429 | -1238.5 | -801.7 | |
| 5.27 | -1.00 | 2.69 | -1.00 | 5.94 | 73.98 | -14.06 | 81.63 | 0.2453 | -1013.0 | 999999 | |
| 3.28 | -1.00 | 1.68 | -1.00 | 5.74 | 73.95 | -14.08 | 82.49 | 0.2453 | -1178.6 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 5.08 | 73.72 | -14.31 | 85.24 | 0.2482 | -838.0 | -558.6 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 5.82 | 73.58 | -14.45 | 82.32 | 0.2517 | -728.0 | -625.6 | |
| 0.00 | 2.16 | 0.00 | 1.11 | 5.25 | 73.53 | -14.50 | 84.59 | 0.2516 | -918.0 | -788.7 | |
| 0.00 | 3.02 | 0.00 | 1.61 | 4.75 | 66.19 | -21.84 | 87.29 | 0.3728 | 950.0 | 833.7 | |
| 0.00 | 1.64 | 0.00 | 0.88 | 4.53 | 66.07 | -21.97 | 87.86 | 0.3748 | 900.0 | 782.2 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 4.71 | 65.93 | -22.10 | 87.40 | 0.3770 | 861.0 | 739.9 | |
| 0.00 | 2.16 | 0.00 | 1.15 | 5.01 | 65.89 | -22.14 | 86.61 | 0.3778 | 773.0 | 650.3 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 5.02 | 65.12 | -22.92 | 86.64 | 0.3903 | 747.0 | 541.0 | |
| 0.00 | 1.30 | 0.00 | 0.70 | 6.32 | 64.87 | -23.17 | 83.35 | 0.3954 | 751.0 | 609.2 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 5.90 | 64.85 | -23.18 | 84.41 | 0.3951 | 808.0 | 677.4 | |
| 0.00 | 3.20 | 0.00 | 1.73 | 6.19 | 64.51 | -23.52 | 83.74 | 0.4008 | 750.0 | 655.0 | |
| 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. | |