SDO HMI 2011-08-31 04:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.53 | 285.76 | 22.30 | 143.27 | 13.91 | 291.44 | -5.70 | 39.12 | 0.1533 | -557.7 | -300.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.25 | 0.00 | 0.63 | 18.36 | 293.21 | -3.94 | 18.55 | 0.2057 | 899.0 | 719.9 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 18.61 | 293.04 | -4.10 | 18.86 | 0.2106 | 830.0 | 631.3 | |
| 43.90 | 262.14 | 21.99 | 131.31 | 13.84 | 291.70 | -5.44 | 38.31 | 0.1492 | -1377.4 | -410.6 | |
| 0.63 | -3.00 | 0.31 | -3.00 | 13.26 | 291.69 | -5.46 | 41.01 | 0.1418 | -1162.0 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 15.75 | 290.71 | -6.44 | 35.77 | 0.1855 | 817.0 | 486.8 | |
| 0.00 | 0.63 | 0.00 | 0.31 | 12.08 | 289.63 | -7.52 | 55.97 | 0.1552 | 915.0 | 696.1 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 12.50 | 289.52 | -7.63 | 54.09 | 0.1607 | 999.0 | 754.5 | |
| 0.00 | 1.88 | 0.00 | 0.95 | 13.56 | 289.30 | -7.85 | 49.76 | 0.1747 | 995.0 | 850.3 | |
| 0.00 | 2.06 | 0.00 | 1.04 | 14.78 | 289.00 | -8.14 | 45.75 | 0.1921 | 874.0 | 695.0 | |
| 0.00 | 2.15 | 0.00 | 1.08 | 11.40 | 289.08 | -8.06 | 61.45 | 0.1573 | 1064.0 | 761.8 | |
| 0.00 | 3.49 | 0.00 | 1.76 | 14.03 | 288.18 | -8.97 | 51.39 | 0.1944 | 800.0 | 724.4 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 14.65 | 287.17 | -9.98 | 51.81 | 0.2142 | 865.0 | 718.3 | |
| 0.00 | 1.25 | 0.00 | 0.64 | 14.50 | 286.99 | -10.16 | 52.89 | 0.2151 | 860.0 | 685.8 | |
| 0.00 | 3.40 | 0.00 | 1.74 | 16.81 | 286.61 | -10.53 | 45.94 | 0.2446 | 887.0 | 693.8 | |
| 0.00 | 2.15 | 0.00 | 1.10 | 16.03 | 286.05 | -11.10 | 49.84 | 0.2432 | 762.0 | 639.3 | |
| 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. | |