SDO HMI 2010-08-11 14:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.73 | 62.07 | 20.99 | 36.49 | 14.28 | 301.36 | -32.15 | 73.46 | 0.5399 | -149.8 | 96.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.28 | 16.15 | 6.51 | 9.32 | 14.07 | 303.09 | -30.43 | 73.26 | 0.5150 | -853.9 | -606.5 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 14.11 | 302.64 | -30.87 | 73.35 | 0.5214 | -412.0 | -337.4 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 14.40 | 302.45 | -31.06 | 72.86 | 0.5250 | 574.0 | 428.2 | |
| 0.00 | 1.44 | 0.00 | 0.84 | 14.11 | 302.20 | -31.31 | 73.49 | 0.5277 | -719.0 | -370.4 | |
| 5.50 | 6.77 | 3.22 | 3.96 | 14.25 | 301.89 | -31.62 | 73.35 | 0.5325 | -833.6 | -612.6 | |
| 1.44 | 1.80 | 0.84 | 1.05 | 13.91 | 301.90 | -31.61 | 73.97 | 0.5314 | -500.1 | -242.8 | |
| 0.00 | 1.80 | 0.00 | 1.06 | 14.11 | 301.65 | -31.86 | 73.68 | 0.5355 | -570.0 | -446.7 | |
| 2.71 | 3.25 | 1.59 | 1.91 | 14.43 | 301.23 | -32.28 | 73.25 | 0.5423 | -639.4 | -504.2 | |
| 2.35 | 3.25 | 1.39 | 1.92 | 14.47 | 300.89 | -32.62 | 73.28 | 0.5472 | -456.6 | -119.8 | |
| 1.35 | 10.47 | 0.80 | 6.19 | 13.69 | 300.79 | -32.72 | 74.72 | 0.5466 | 847.2 | 589.2 | |
| 1.44 | -10.00 | 0.85 | -10.00 | 13.90 | 300.61 | -32.90 | 74.40 | 0.5496 | 764.9 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.75 | 14.70 | 300.06 | -33.45 | 73.14 | 0.5593 | 742.0 | 565.1 | |
| 9.66 | 11.55 | 5.79 | 6.93 | 15.08 | 299.69 | -33.82 | 72.60 | 0.5654 | 789.7 | 568.6 | |
| 0.00 | 2.62 | 0.00 | 1.57 | 13.92 | 299.44 | -34.07 | 74.69 | 0.5660 | 756.0 | 606.2 | |
| 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. | |