SDO HMI 2014-11-30 16:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.44 | 53.13 | 11.34 | 28.08 | -19.06 | 108.29 | 3.54 | 189.60 | 0.3498 | 292.8 | 86.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.47 | 21.79 | 2.90 | 11.55 | -19.31 | 109.81 | 5.06 | 193.52 | 0.3579 | 1034.0 | 492.0 | |
| 0.00 | 1.37 | 0.00 | 0.73 | -19.63 | 109.72 | 4.98 | 193.09 | 0.3626 | 784.0 | 643.7 | |
| 9.91 | -1.00 | 5.25 | -1.00 | -19.37 | 109.50 | 4.75 | 192.67 | 0.3577 | 967.3 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -19.66 | 109.50 | 4.76 | 192.51 | 0.3623 | 602.0 | 539.4 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -19.28 | 109.05 | 4.31 | 191.59 | 0.3547 | 709.0 | 565.8 | |
| 0.85 | 2.73 | 0.45 | 1.44 | -18.87 | 108.70 | 3.95 | 190.89 | 0.3469 | -651.8 | -435.3 | |
| 1.54 | 8.54 | 0.81 | 4.51 | -18.96 | 108.17 | 3.42 | 189.41 | 0.3469 | 1126.7 | 774.2 | |
| 2.56 | 5.38 | 1.34 | 2.82 | -18.08 | 107.68 | 2.94 | 188.50 | 0.3314 | -1027.3 | -805.6 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -17.67 | 106.65 | 1.91 | 185.67 | 0.3225 | 873.0 | 677.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -19.24 | 106.64 | 1.89 | 185.16 | 0.3483 | -872.0 | -701.2 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -18.77 | 106.60 | 1.86 | 185.19 | 0.3405 | -786.0 | -483.0 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -18.93 | 106.29 | 1.55 | 184.29 | 0.3426 | 263.0 | 279.9 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -18.74 | 105.95 | 1.20 | 183.37 | 0.3391 | -640.0 | -356.5 | |
| 1.11 | 4.19 | 0.59 | 2.21 | -19.27 | 105.20 | 0.45 | 181.24 | 0.3474 | -936.4 | -857.2 | |
| 0.00 | 2.05 | 0.00 | 1.08 | -18.92 | 105.10 | 0.36 | 181.00 | 0.3417 | -800.0 | -700.8 | |
| 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. | |