SDO HMI 2011-06-07 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.73 | 64.69 | 13.67 | 49.41 | 17.14 | 19.93 | 47.20 | 292.78 | 0.7621 | -221.9 | -221.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.98 | 17.28 | 3.92 | 13.59 | 17.02 | 21.60 | 48.87 | 292.05 | 0.7793 | -520.4 | -239.8 | |
| 3.80 | 28.50 | 2.94 | 22.01 | 16.70 | 20.82 | 48.08 | 291.89 | 0.7704 | -647.3 | -501.9 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 18.30 | 21.39 | 48.65 | 293.70 | 0.7807 | -313.0 | -281.0 | |
| 0.00 | 1.00 | 0.00 | 0.77 | 17.02 | 20.69 | 47.95 | 292.33 | 0.7699 | -441.0 | -460.0 | |
| 4.61 | -2.00 | 3.54 | -2.00 | 16.67 | 20.43 | 47.69 | 291.97 | 0.7662 | -845.2 | 999999 | |
| 1.90 | 3.44 | 1.51 | 2.72 | 19.36 | 21.26 | 48.53 | 295.06 | 0.7826 | 208.8 | 277.2 | |
| 1.45 | 1.90 | 1.06 | 1.39 | 16.83 | 17.66 | 44.93 | 293.11 | 0.7372 | -629.8 | -643.4 | |
| 0.00 | 1.99 | 0.00 | 1.44 | 17.02 | 17.04 | 44.31 | 293.58 | 0.7311 | -749.0 | -624.1 | |
| 0.00 | 0.90 | 0.00 | 0.65 | 18.82 | 15.60 | 42.87 | 296.52 | 0.7220 | 466.0 | 391.4 | |
| 0.00 | 2.62 | 0.00 | 1.85 | 17.60 | 15.19 | 42.46 | 295.08 | 0.7127 | 638.0 | 507.0 | |
| 0.54 | 5.43 | 0.38 | 3.82 | 17.76 | 15.10 | 42.37 | 295.33 | 0.7124 | 822.7 | 541.8 | |
| 0.45 | -11.00 | 0.32 | -11.00 | 17.85 | 15.00 | 42.27 | 295.50 | 0.7116 | 805.8 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.96 | 18.94 | 15.16 | 42.43 | 296.88 | 0.7177 | 678.0 | 523.9 | |
| 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. | |