SDO HMI 2011-10-11 20:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 113.82 | 607.49 | 89.68 | 477.45 | 26.88 | 58.31 | -48.83 | 60.04 | 0.7770 | -911.0 | -265.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 588.86 | 0.26 | 461.10 | 26.47 | 60.39 | -46.74 | 59.92 | 0.7557 | 78.8 | -279.1 | |
| 2.27 | -1.00 | 1.72 | -1.00 | 26.43 | 60.31 | -46.82 | 59.99 | 0.7564 | -306.8 | 999999 | |
| 1.22 | -1.00 | 0.93 | -1.00 | 26.64 | 60.10 | -47.03 | 59.79 | 0.7591 | -826.4 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.53 | 24.89 | 60.03 | -47.10 | 62.05 | 0.7545 | 543.0 | 435.4 | |
| 100.80 | -1.00 | 78.74 | -1.00 | 26.98 | 58.51 | -48.63 | 59.87 | 0.7755 | -1139.9 | 999999 | |
| 4.81 | -1.00 | 3.85 | -1.00 | 27.51 | 57.31 | -49.82 | 59.57 | 0.7882 | -283.2 | 999999 | |
| 0.96 | -1.00 | 0.77 | -1.00 | 27.07 | 57.53 | -49.61 | 60.05 | 0.7850 | -195.7 | 999999 | |
| 0.35 | -1.00 | 0.28 | -1.00 | 26.56 | 57.77 | -49.36 | 60.60 | 0.7813 | -610.8 | 999999 | |
| 0.00 | 4.90 | 0.00 | 3.81 | 24.95 | 58.17 | -48.96 | 62.52 | 0.7732 | 317.0 | 357.5 | |
| 0.00 | 1.14 | 0.00 | 0.89 | 24.78 | 58.06 | -49.07 | 62.76 | 0.7738 | 410.0 | 450.8 | |
| 0.00 | 0.61 | 0.00 | 0.50 | 26.86 | 56.50 | -50.63 | 60.60 | 0.7940 | -236.0 | -178.6 | |
| 0.00 | 1.31 | 0.00 | 1.00 | 20.05 | 57.94 | -49.19 | 68.84 | 0.7647 | -626.0 | -423.7 | |
| 0.00 | 0.96 | 0.00 | 0.82 | 26.52 | 53.98 | -53.15 | 61.63 | 0.8159 | -403.0 | -309.1 | |
| 0.00 | 1.14 | 0.00 | 0.89 | 20.45 | 56.77 | -50.36 | 68.54 | 0.7776 | -452.0 | -386.9 | |
| 0.00 | 1.75 | 0.00 | 1.54 | 25.67 | 52.34 | -54.79 | 63.00 | 0.8286 | -509.0 | -367.5 | |
| 3.06 | 4.55 | 3.13 | 4.66 | 23.58 | 46.14 | -60.99 | 66.40 | 0.8767 | 542.9 | 427.2 | |
| 0.00 | 1.57 | 0.00 | 1.71 | 23.30 | 44.13 | -63.01 | 66.92 | 0.8915 | 514.0 | 463.5 | |
| 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. | |