SDO HMI 2010-08-12 02:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.68 | 67.75 | 16.32 | 37.24 | 14.17 | 302.01 | -24.87 | 70.52 | 0.4341 | -66.1 | -311.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.41 | 12.00 | 2.92 | 6.49 | 14.14 | 304.30 | -22.58 | 69.19 | 0.4000 | -1076.2 | -852.9 | |
| 0.00 | 1.53 | 0.00 | 0.83 | 13.92 | 303.44 | -23.44 | 70.29 | 0.4119 | -845.0 | -626.8 | |
| 3.07 | 16.15 | 1.67 | 8.81 | 14.17 | 302.90 | -23.98 | 70.04 | 0.4210 | -957.9 | -835.4 | |
| 2.80 | -3.00 | 1.53 | -3.00 | 14.38 | 302.81 | -24.08 | 69.62 | 0.4233 | -811.8 | 999999 | |
| 5.14 | 7.94 | 2.82 | 4.36 | 14.33 | 302.30 | -24.59 | 70.06 | 0.4306 | -837.7 | -504.8 | |
| 0.00 | 3.25 | 0.00 | 1.78 | 13.99 | 302.20 | -24.69 | 70.88 | 0.4307 | -677.0 | -652.1 | |
| 0.00 | 2.08 | 0.00 | 1.14 | 13.69 | 301.78 | -25.10 | 71.78 | 0.4357 | -606.0 | -501.7 | |
| 10.29 | 12.27 | 5.71 | 6.81 | 13.60 | 300.61 | -26.27 | 72.56 | 0.4528 | 1003.0 | 775.9 | |
| 0.00 | 1.71 | 0.00 | 0.95 | 13.78 | 300.38 | -26.50 | 72.30 | 0.4568 | 380.0 | 337.3 | |
| 0.00 | 1.80 | 0.00 | 1.01 | 14.72 | 300.12 | -26.76 | 70.43 | 0.4641 | 804.0 | 647.5 | |
| 1.17 | 7.58 | 0.66 | 4.25 | 15.11 | 299.86 | -27.03 | 69.77 | 0.4694 | 841.1 | 731.1 | |
| 1.80 | -11.00 | 1.01 | -11.00 | 15.03 | 299.62 | -27.26 | 70.05 | 0.4726 | 668.5 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.81 | 13.80 | 299.57 | -27.31 | 72.63 | 0.4688 | 858.0 | 645.2 | |
| 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. | |