SDO HMI 2014-11-29 18:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.20 | 450.91 | 40.41 | 233.31 | 16.49 | 110.38 | -6.43 | 21.92 | 0.2885 | -1029.0 | -341.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.83 | 431.84 | 39.70 | 223.30 | 16.48 | 110.60 | -6.21 | 21.34 | 0.2865 | -1540.7 | -387.9 | |
| 1.37 | -1.00 | 0.71 | -1.00 | 16.45 | 109.77 | -7.05 | 23.94 | 0.2914 | -900.4 | 999999 | |
| 0.00 | 2.48 | 0.00 | 1.27 | 14.65 | 109.24 | -7.58 | 28.52 | 0.2683 | -886.0 | -621.8 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 17.80 | 108.21 | -8.61 | 26.33 | 0.3226 | 646.0 | 396.2 | |
| 0.00 | 3.25 | 0.00 | 1.70 | 17.33 | 106.98 | -9.84 | 30.21 | 0.3256 | 898.0 | 821.9 | |
| 0.00 | 3.42 | 0.00 | 1.79 | 17.55 | 106.87 | -9.94 | 30.12 | 0.3295 | 887.0 | 758.0 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 17.76 | 104.78 | -12.04 | 34.66 | 0.3510 | 842.0 | 689.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 17.45 | 104.73 | -12.09 | 35.28 | 0.3473 | 898.0 | 626.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.33 | 104.23 | -12.58 | 36.58 | 0.3505 | 620.0 | 545.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 17.21 | 103.99 | -12.83 | 37.33 | 0.3514 | 710.0 | 519.5 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 16.00 | 102.55 | -14.27 | 42.55 | 0.3519 | 749.0 | 593.3 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 15.39 | 102.59 | -14.23 | 43.72 | 0.3443 | 818.0 | 661.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 15.91 | 102.18 | -14.64 | 43.46 | 0.3550 | 857.0 | 660.9 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 15.54 | 101.76 | -15.06 | 45.00 | 0.3556 | 840.0 | 690.1 | |
| 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. | |