SDO HMI 2011-06-01 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.49 | 73.98 | 12.64 | 39.79 | 17.19 | 41.90 | -14.11 | 36.79 | 0.3882 | -324.4 | -159.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.53 | 0.00 | 1.33 | 18.09 | 48.50 | -7.51 | 21.16 | 0.3459 | 972.0 | 736.7 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 15.90 | 46.77 | -9.25 | 28.50 | 0.3253 | 510.0 | 423.3 | |
| 5.24 | 40.47 | 2.80 | 21.62 | 17.75 | 43.79 | -12.23 | 32.61 | 0.3760 | -1100.7 | -418.6 | |
| 3.25 | -3.00 | 1.74 | -3.00 | 17.62 | 43.57 | -12.45 | 33.26 | 0.3762 | -998.6 | 999999 | |
| 6.87 | -3.00 | 3.66 | -3.00 | 17.05 | 43.38 | -12.64 | 34.56 | 0.3704 | -1024.3 | 999999 | |
| 0.63 | 2.62 | 0.34 | 1.40 | 16.73 | 42.98 | -13.04 | 35.91 | 0.3700 | -957.0 | -662.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 15.69 | 41.94 | -14.07 | 39.81 | 0.3672 | -832.0 | -604.8 | |
| 2.80 | 3.43 | 1.50 | 1.83 | 16.10 | 41.52 | -14.49 | 39.88 | 0.3766 | -897.8 | -806.0 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 15.85 | 41.35 | -14.67 | 40.67 | 0.3755 | -928.0 | -831.3 | |
| 0.00 | 3.43 | 0.00 | 1.84 | 16.04 | 41.27 | -14.75 | 40.48 | 0.3786 | -772.0 | -691.9 | |
| 0.00 | 1.72 | 0.00 | 0.92 | 15.41 | 40.10 | -15.91 | 43.75 | 0.3839 | -830.0 | -657.0 | |
| 3.16 | 5.06 | 1.74 | 2.78 | 17.45 | 37.59 | -18.43 | 44.19 | 0.4343 | 859.3 | 817.1 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 16.75 | 36.89 | -19.12 | 46.43 | 0.4348 | 802.0 | 553.8 | |
| 0.00 | 3.07 | 0.00 | 1.72 | 19.26 | 36.33 | -19.68 | 43.10 | 0.4673 | 908.0 | 667.2 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 17.49 | 35.36 | -20.66 | 47.29 | 0.4599 | 769.0 | 556.0 | |
| 1.54 | 3.07 | 0.86 | 1.71 | 17.02 | 35.00 | -21.02 | 48.56 | 0.4593 | 828.5 | 706.8 | |
| 0.00 | 1.26 | 0.00 | 0.71 | 17.27 | 34.90 | -21.11 | 48.26 | 0.4629 | 721.0 | 571.5 | |
| 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. | |