SDO HMI 2014-11-27 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 |
| 60.48 | 366.51 | 37.20 | 226.31 | 16.10 | 110.34 | -33.95 | 64.24 | 0.5977 | -800.7 | -302.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.08 | 352.05 | 35.69 | 216.63 | 16.08 | 110.63 | -33.65 | 64.13 | 0.5940 | -1272.8 | -342.3 | |
| 1.97 | -1.00 | 1.22 | -1.00 | 16.50 | 109.95 | -34.33 | 63.85 | 0.6046 | -583.7 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.87 | 16.42 | 108.08 | -36.20 | 64.98 | 0.6276 | -535.0 | -353.4 | |
| 0.00 | 1.03 | 0.00 | 0.66 | 16.41 | 107.50 | -36.78 | 65.27 | 0.6346 | 839.0 | 608.9 | |
| 0.00 | 1.45 | 0.00 | 0.94 | 16.56 | 107.08 | -37.20 | 65.26 | 0.6404 | 790.0 | 693.4 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 16.32 | 105.25 | -39.03 | 66.44 | 0.6617 | 751.0 | 634.3 | |
| 0.00 | 1.20 | 0.00 | 0.80 | 16.13 | 104.54 | -39.75 | 67.02 | 0.6695 | 558.0 | 421.1 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 15.36 | 104.68 | -39.61 | 68.07 | 0.6650 | 517.0 | 356.7 | |
| 0.00 | 1.20 | 0.00 | 0.81 | 16.82 | 103.35 | -40.93 | 66.53 | 0.6861 | 622.0 | 565.1 | |
| 0.43 | 1.71 | 0.29 | 1.17 | 16.38 | 102.68 | -41.60 | 67.40 | 0.6923 | 767.8 | 696.1 | |
| 0.00 | 1.97 | 0.00 | 1.35 | 16.47 | 102.37 | -41.91 | 67.40 | 0.6963 | 480.0 | 413.1 | |
| 0.00 | 0.68 | 0.00 | 0.47 | 16.00 | 102.12 | -42.17 | 68.13 | 0.6977 | 631.0 | 572.9 | |
| 0.00 | 1.54 | 0.00 | 1.07 | 15.78 | 101.80 | -42.49 | 68.55 | 0.7007 | 801.0 | 559.7 | |
| 0.00 | 0.34 | 0.00 | 0.24 | 15.72 | 101.48 | -42.80 | 68.75 | 0.7042 | 300.0 | 331.8 | |
| 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. | |