SDO HMI 2011-10-05 02:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.40 | 372.54 | 43.67 | 248.70 | 23.21 | 156.00 | -40.18 | 62.28 | 0.6720 | -770.2 | -304.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.67 | 0.00 | 1.12 | 26.62 | 156.65 | -39.54 | 57.21 | 0.6793 | -797.0 | -631.5 | |
| 15.56 | 293.97 | 10.26 | 194.62 | 22.63 | 156.70 | -39.48 | 62.83 | 0.6619 | -1134.3 | -367.9 | |
| 0.00 | 1.05 | 0.00 | 0.72 | 26.01 | 155.32 | -40.86 | 58.64 | 0.6908 | -525.0 | -423.2 | |
| 29.36 | -2.00 | 19.50 | -2.00 | 23.18 | 156.34 | -39.84 | 62.19 | 0.6681 | -1098.0 | 999999 | |
| 1.58 | -2.00 | 1.05 | -2.00 | 22.27 | 156.41 | -39.78 | 63.48 | 0.6640 | -767.8 | 999999 | |
| 3.25 | -2.00 | 2.16 | -2.00 | 22.43 | 156.09 | -40.09 | 63.36 | 0.6682 | -607.3 | 999999 | |
| 14.42 | 64.26 | 9.80 | 43.86 | 24.13 | 154.99 | -41.19 | 61.38 | 0.6870 | -918.8 | -131.8 | |
| 0.00 | 1.05 | 0.00 | 0.70 | 21.60 | 155.40 | -40.78 | 64.82 | 0.6734 | -278.0 | -267.8 | |
| 0.00 | 1.41 | 0.00 | 0.95 | 22.79 | 154.93 | -41.25 | 63.28 | 0.6828 | -129.0 | -66.2 | |
| 0.00 | 0.79 | 0.00 | 0.52 | 19.83 | 155.60 | -40.58 | 67.33 | 0.6655 | 691.0 | 537.6 | |
| 0.00 | 0.26 | 0.00 | 0.18 | 22.04 | 154.56 | -41.62 | 64.49 | 0.6845 | -369.0 | -317.0 | |
| 0.00 | 0.88 | 0.00 | 0.61 | 22.72 | 152.66 | -43.52 | 64.17 | 0.7080 | 615.0 | 521.2 | |
| 1.23 | 1.93 | 0.90 | 1.41 | 24.72 | 150.45 | -45.73 | 62.18 | 0.7377 | 618.8 | 431.4 | |
| 0.00 | 0.79 | 0.00 | 0.60 | 26.45 | 148.70 | -47.49 | 60.48 | 0.7607 | 558.0 | 488.3 | |
| 0.00 | 2.20 | 0.00 | 1.67 | 26.16 | 148.66 | -47.52 | 60.87 | 0.7602 | 632.0 | 515.1 | |
| 0.00 | 0.79 | 0.00 | 0.60 | 25.42 | 148.80 | -47.38 | 61.77 | 0.7567 | 575.0 | 528.4 | |
| 0.00 | 1.49 | 0.00 | 1.14 | 25.06 | 147.90 | -48.28 | 62.49 | 0.7647 | 536.0 | 439.8 | |
| 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. | |