SDO HMI 2014-11-29 12:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.30 | 26.86 | 3.30 | 16.30 | 16.72 | 152.29 | 32.17 | 298.13 | 0.5802 | 117.1 | -13.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.53 | 6.93 | 2.83 | 4.33 | 17.26 | 154.63 | 34.51 | 297.49 | 0.6122 | 834.8 | 614.6 | |
| 0.77 | 2.14 | 0.47 | 1.30 | 15.43 | 152.90 | 32.77 | 295.65 | 0.5811 | 778.1 | 633.6 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 15.19 | 152.74 | 32.62 | 295.35 | 0.5779 | 674.0 | 522.6 | |
| 0.00 | 1.62 | 0.00 | 0.98 | 15.59 | 152.45 | 32.33 | 296.17 | 0.5761 | 825.0 | 741.5 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 15.47 | 152.28 | 32.16 | 296.08 | 0.5734 | 256.0 | 289.5 | |
| 0.00 | 2.82 | 0.00 | 1.71 | 16.70 | 152.25 | 32.13 | 298.08 | 0.5796 | 690.0 | 587.3 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 16.42 | 152.20 | 32.08 | 297.67 | 0.5774 | 615.0 | 541.2 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 17.23 | 151.12 | 31.00 | 299.70 | 0.5685 | -826.0 | -692.5 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 17.51 | 150.70 | 30.58 | 300.45 | 0.5650 | -612.0 | -453.6 | |
| 0.00 | 4.02 | 0.00 | 2.39 | 16.50 | 150.48 | 30.36 | 298.96 | 0.5560 | -832.0 | -696.4 | |
| 0.00 | 1.80 | 0.00 | 1.07 | 17.39 | 150.46 | 30.34 | 300.43 | 0.5612 | -785.0 | -597.3 | |
| 0.00 | 1.71 | 0.00 | 1.02 | 17.21 | 150.32 | 30.20 | 300.23 | 0.5583 | -944.0 | -733.7 | |
| 0.00 | 1.28 | 0.00 | 0.77 | 17.80 | 150.39 | 30.27 | 301.13 | 0.5629 | -775.0 | -606.5 | |
| 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. | |