SDO HMI 2011-06-07 11:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.85 | 139.76 | 16.49 | 70.33 | 9.75 | 336.45 | -1.27 | 6.28 | 0.1719 | -770.1 | -407.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.72 | 0.00 | 0.86 | 7.87 | 339.45 | 1.73 | 347.55 | 0.1397 | -997.0 | -776.2 | |
| 0.00 | 1.90 | 0.00 | 0.96 | 11.17 | 337.92 | 0.20 | 358.98 | 0.1935 | -752.0 | -559.9 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 8.40 | 337.15 | -0.57 | 3.88 | 0.1458 | -779.0 | -518.3 | |
| 29.23 | 116.21 | 14.68 | 58.38 | 9.50 | 336.93 | -0.79 | 4.72 | 0.1652 | -1351.4 | -446.9 | |
| 1.45 | 3.71 | 0.72 | 1.86 | 7.94 | 336.38 | -1.34 | 9.58 | 0.1394 | -950.4 | -890.9 | |
| 2.17 | 2.53 | 1.09 | 1.27 | 8.77 | 336.19 | -1.52 | 9.87 | 0.1541 | -873.7 | -1030.8 | |
| 0.00 | 3.35 | 0.00 | 1.68 | 8.21 | 335.52 | -2.20 | 15.01 | 0.1473 | -1072.0 | -802.3 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 10.65 | 335.22 | -2.49 | 13.11 | 0.1893 | -882.0 | -671.3 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 11.98 | 330.87 | -6.84 | 29.45 | 0.2381 | 741.0 | 630.7 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.99 | 330.34 | -7.38 | 24.23 | 0.3022 | 845.0 | 685.8 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 14.86 | 329.52 | -8.19 | 28.36 | 0.2913 | 742.0 | 575.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 14.76 | 329.17 | -8.54 | 29.52 | 0.2928 | 809.0 | 613.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 17.71 | 326.25 | -11.46 | 31.99 | 0.3588 | 891.0 | 722.9 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 20.42 | 322.93 | -14.79 | 34.53 | 0.4238 | 760.0 | 574.6 | |
| 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. | |