SDO HMI 2011-06-02 17:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.85 | 285.21 | 20.90 | 158.04 | 16.93 | 20.31 | -20.26 | 47.77 | 0.4482 | -338.7 | -332.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.80 | 18.44 | 22.08 | -18.50 | 42.85 | 0.4444 | -874.0 | -796.7 | |
| 0.00 | 1.72 | 0.00 | 0.96 | 18.73 | 21.12 | -19.45 | 43.76 | 0.4577 | -767.0 | -600.8 | |
| 19.15 | 241.05 | 10.52 | 132.52 | 16.49 | 21.31 | -19.26 | 47.28 | 0.4323 | -1272.7 | -456.5 | |
| 0.90 | -3.00 | 0.50 | -3.00 | 16.11 | 21.25 | -19.32 | 48.05 | 0.4292 | -1102.9 | 999999 | |
| 3.61 | -3.00 | 1.99 | -3.00 | 17.00 | 21.09 | -19.49 | 46.70 | 0.4401 | -1073.8 | 999999 | |
| 2.17 | -3.00 | 1.20 | -3.00 | 17.16 | 20.93 | -19.64 | 46.64 | 0.4435 | -858.3 | 999999 | |
| 4.43 | -3.00 | 2.44 | -3.00 | 16.59 | 20.93 | -19.64 | 47.65 | 0.4377 | -1063.5 | 999999 | |
| 2.26 | -3.00 | 1.25 | -3.00 | 16.85 | 20.77 | -19.81 | 47.43 | 0.4422 | -932.2 | 999999 | |
| 1.08 | -3.00 | 0.60 | -3.00 | 16.50 | 20.74 | -19.83 | 48.08 | 0.4390 | -856.8 | 999999 | |
| 1.36 | -3.00 | 0.75 | -3.00 | 16.62 | 20.59 | -19.98 | 48.06 | 0.4420 | -655.7 | 999999 | |
| 1.72 | -3.00 | 0.95 | -3.00 | 16.37 | 20.61 | -19.96 | 48.48 | 0.4392 | -656.2 | 999999 | |
| 0.00 | 4.52 | 0.00 | 2.54 | 19.03 | 19.99 | -20.58 | 44.85 | 0.4731 | -573.0 | -572.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 18.42 | 19.93 | -20.64 | 45.91 | 0.4675 | -626.0 | -547.3 | |
| 0.00 | 1.81 | 0.00 | 1.01 | 18.19 | 19.72 | -20.85 | 46.55 | 0.4676 | -657.0 | -518.5 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 17.81 | 19.46 | -21.11 | 47.53 | 0.4667 | -760.0 | -644.8 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 17.71 | 19.30 | -21.27 | 47.89 | 0.4676 | -687.0 | -570.6 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 17.62 | 18.18 | -22.39 | 49.44 | 0.4798 | -728.0 | -613.2 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 18.40 | 16.78 | -23.79 | 49.80 | 0.5031 | 787.0 | 658.9 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 18.53 | 16.38 | -24.19 | 50.04 | 0.5089 | -612.0 | -612.0 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 19.14 | 16.25 | -24.32 | 49.22 | 0.5159 | 759.0 | 538.4 | |
| 0.00 | 1.26 | 0.00 | 0.74 | 19.69 | 15.56 | -25.02 | 49.11 | 0.5287 | 816.0 | 629.3 | |
| 0.00 | 1.17 | 0.00 | 0.70 | 21.23 | 14.71 | -25.86 | 47.73 | 0.5517 | 733.0 | 600.7 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 17.95 | 15.20 | -25.37 | 52.22 | 0.5179 | 793.0 | 649.4 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 16.36 | 15.32 | -25.25 | 54.73 | 0.5033 | 912.0 | 740.4 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 21.52 | 14.47 | -26.10 | 47.55 | 0.5569 | 740.0 | 633.4 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 17.73 | 15.05 | -25.52 | 52.72 | 0.5177 | 902.0 | 693.6 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 19.66 | 14.67 | -25.91 | 50.08 | 0.5385 | 782.0 | 663.3 | |
| 0.00 | 2.44 | 0.00 | 1.40 | 16.58 | 14.98 | -25.59 | 54.69 | 0.5093 | 840.0 | 700.0 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 17.51 | 14.70 | -25.87 | 53.44 | 0.5201 | 699.0 | 443.8 | |
| 0.00 | 2.35 | 0.00 | 1.41 | 21.69 | 13.81 | -26.76 | 47.97 | 0.5654 | 731.0 | 593.8 | |
| 0.00 | 4.61 | 0.00 | 2.72 | 19.25 | 13.73 | -26.84 | 51.65 | 0.5457 | 846.0 | 843.4 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 20.87 | 13.39 | -27.18 | 49.55 | 0.5630 | 508.0 | 404.5 | |
| 0.00 | 1.17 | 0.00 | 0.69 | 18.93 | 13.35 | -27.22 | 52.50 | 0.5474 | 864.0 | 633.6 | |
| 1.17 | 3.07 | 0.70 | 1.82 | 19.22 | 13.23 | -27.34 | 52.17 | 0.5512 | 676.3 | 621.7 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 18.70 | 13.32 | -27.25 | 52.88 | 0.5460 | 789.0 | 717.1 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 14.66 | 13.06 | -27.51 | 59.73 | 0.5195 | 684.0 | 455.7 | |
| 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. | |