SDO HMI 2011-09-04 07:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.60 | 139.78 | 23.82 | 139.57 | 23.21 | 303.22 | 60.55 | 292.81 | 0.8680 | -165.4 | -64.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.43 | 109.00 | 1.52 | 114.60 | 22.53 | 305.57 | 62.90 | 291.69 | 0.8869 | 263.2 | -181.0 | |
| 17.79 | -1.00 | 18.71 | -1.00 | 22.64 | 305.16 | 62.49 | 291.85 | 0.8838 | -779.0 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.57 | 25.10 | 299.63 | 56.96 | 295.29 | 0.8417 | -506.0 | -411.4 | |
| 0.00 | 2.06 | 0.00 | 1.69 | 25.07 | 295.02 | 52.35 | 296.06 | 0.8005 | 397.0 | 365.0 | |
| 0.00 | 1.52 | 0.00 | 1.26 | 25.65 | 295.38 | 52.71 | 296.70 | 0.8050 | 439.0 | 357.6 | |
| 1.52 | 1.88 | 1.25 | 1.55 | 25.52 | 295.02 | 52.35 | 296.62 | 0.8014 | 413.9 | 319.5 | |
| 0.00 | 2.06 | 0.00 | 1.68 | 25.09 | 294.76 | 52.09 | 296.14 | 0.7981 | 646.0 | 602.4 | |
| 0.00 | 1.61 | 0.00 | 1.32 | 25.82 | 294.71 | 52.04 | 297.05 | 0.7991 | 448.0 | 380.6 | |
| 0.00 | 1.25 | 0.00 | 1.03 | 26.60 | 294.76 | 52.09 | 297.99 | 0.8012 | 362.0 | 248.6 | |
| 1.07 | 2.77 | 0.87 | 2.25 | 25.84 | 294.12 | 51.45 | 297.20 | 0.7937 | 564.1 | 424.6 | |
| 1.79 | 3.22 | 1.47 | 2.64 | 26.65 | 294.52 | 51.85 | 298.12 | 0.7991 | 519.7 | 387.9 | |
| 0.00 | 2.24 | 0.00 | 1.80 | 25.64 | 293.79 | 51.12 | 297.03 | 0.7901 | 714.0 | 608.4 | |
| 0.00 | 1.97 | 0.00 | 1.56 | 25.24 | 293.18 | 50.51 | 296.67 | 0.7834 | 673.0 | 523.5 | |
| 0.00 | 3.22 | 0.00 | 2.58 | 26.21 | 293.59 | 50.93 | 297.79 | 0.7895 | 516.0 | 454.2 | |
| 0.00 | 1.79 | 0.00 | 1.42 | 25.83 | 293.15 | 50.48 | 297.42 | 0.7845 | 610.0 | 607.2 | |
| 0.00 | 2.15 | 0.00 | 1.72 | 26.80 | 293.26 | 50.59 | 298.60 | 0.7877 | 645.0 | 502.5 | |
| 0.00 | 1.16 | 0.00 | 0.92 | 26.28 | 292.84 | 50.17 | 298.06 | 0.7825 | 818.0 | 666.3 | |
| 0.00 | 1.25 | 0.00 | 0.98 | 26.26 | 292.08 | 49.42 | 298.22 | 0.7752 | 549.0 | 470.1 | |
| 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. | |