SDO HMI 2014-11-01 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.13 | 82.43 | 13.36 | 42.16 | 12.77 | 114.90 | -11.59 | 52.78 | 0.2471 | -460.1 | -166.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.73 | 54.16 | 0.88 | 27.64 | 13.17 | 115.55 | -10.94 | 50.01 | 0.2422 | -1041.6 | -387.1 | |
| 16.70 | -1.00 | 8.52 | -1.00 | 12.84 | 115.54 | -10.95 | 51.14 | 0.2390 | -1289.6 | 999999 | |
| 2.25 | -1.00 | 1.15 | -1.00 | 13.10 | 114.96 | -11.52 | 51.65 | 0.2492 | -520.3 | 999999 | |
| 0.00 | 3.29 | 0.00 | 1.68 | 12.68 | 114.92 | -11.57 | 53.14 | 0.2456 | 74.0 | 56.1 | |
| 1.64 | 5.88 | 0.84 | 3.00 | 11.93 | 114.89 | -11.60 | 55.79 | 0.2389 | -921.1 | -616.9 | |
| 0.52 | 1.73 | 0.27 | 0.89 | 13.31 | 114.39 | -12.10 | 52.31 | 0.2589 | -835.5 | -627.1 | |
| 0.00 | 2.16 | 0.00 | 1.11 | 11.98 | 114.33 | -12.16 | 56.81 | 0.2473 | 805.0 | 480.8 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 12.46 | 114.28 | -12.21 | 55.29 | 0.2524 | 54.0 | 149.5 | |
| 2.08 | 3.89 | 1.07 | 2.00 | 13.23 | 113.40 | -13.09 | 54.63 | 0.2717 | -521.0 | -300.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 11.82 | 113.47 | -13.02 | 59.07 | 0.2583 | 826.0 | 722.8 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 12.90 | 113.35 | -13.14 | 55.75 | 0.2693 | 870.0 | 647.8 | |
| 0.00 | 2.42 | 0.00 | 1.25 | 12.71 | 113.02 | -13.47 | 56.97 | 0.2723 | 1176.0 | 930.2 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 11.91 | 111.93 | -14.56 | 61.37 | 0.2815 | 628.0 | 423.9 | |
| 1.21 | 2.42 | 0.63 | 1.26 | 12.81 | 111.44 | -15.05 | 59.38 | 0.2956 | 1006.0 | 777.9 | |
| 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. | |