SDO HMI 2011-05-29 00:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.77 | 20.74 | 3.01 | 10.87 | -16.34 | 114.19 | 11.33 | 215.30 | 0.3262 | -225.4 | -50.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.53 | -17.64 | 117.35 | 14.50 | 219.88 | 0.3737 | 732.0 | 524.4 | |
| 0.00 | 2.08 | 0.00 | 1.10 | -17.10 | 117.28 | 14.42 | 220.73 | 0.3664 | 896.0 | 681.5 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -16.47 | 116.87 | 14.01 | 221.13 | 0.3545 | 687.0 | 618.5 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -16.00 | 116.57 | 13.72 | 221.47 | 0.3457 | 829.0 | 581.7 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -15.75 | 116.10 | 13.25 | 221.00 | 0.3376 | 795.0 | 640.4 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -16.54 | 115.41 | 12.55 | 217.97 | 0.3401 | 649.0 | 610.1 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -16.86 | 114.00 | 11.15 | 214.20 | 0.3306 | -733.0 | -534.8 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -17.59 | 113.59 | 10.74 | 211.98 | 0.3368 | -714.0 | -537.0 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -15.63 | 112.97 | 10.11 | 213.91 | 0.3044 | -885.0 | -658.1 | |
| 0.00 | 1.62 | 0.00 | 0.85 | -15.85 | 112.98 | 10.13 | 213.52 | 0.3075 | -876.0 | -574.3 | |
| 0.72 | 1.99 | 0.38 | 1.03 | -15.79 | 112.66 | 9.80 | 212.80 | 0.3037 | -1120.1 | -964.4 | |
| 0.72 | 6.59 | 0.38 | 3.43 | -16.30 | 112.58 | 9.73 | 211.70 | 0.3101 | -741.1 | -709.7 | |
| 4.33 | -12.00 | 2.25 | -12.00 | -16.14 | 112.48 | 9.63 | 211.70 | 0.3070 | -975.5 | 999999 | |
| 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. | |