SDO HMI 2011-07-17 22:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.65 | 262.20 | 19.72 | 133.98 | 16.83 | 168.91 | 6.72 | 331.73 | 0.2436 | -815.1 | -364.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.60 | 10.06 | 172.10 | 9.91 | 299.79 | 0.1960 | -789.0 | -555.6 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 12.46 | 172.02 | 9.83 | 309.70 | 0.2177 | -763.0 | -581.6 | |
| 1.27 | 242.70 | 0.65 | 123.83 | 16.88 | 169.33 | 7.14 | 330.93 | 0.2458 | -964.0 | -444.6 | |
| 28.85 | -3.00 | 14.72 | -3.00 | 16.54 | 169.25 | 7.06 | 330.48 | 0.2402 | -1331.9 | 999999 | |
| 7.71 | -3.00 | 3.93 | -3.00 | 16.17 | 169.17 | 6.98 | 329.93 | 0.2341 | -1416.6 | 999999 | |
| 0.82 | -3.00 | 0.42 | -3.00 | 16.36 | 168.77 | 6.57 | 331.80 | 0.2335 | -1023.9 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.45 | 168.29 | 6.10 | 335.60 | 0.2465 | -714.0 | -549.7 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 21.12 | 166.07 | 3.88 | 347.53 | 0.2933 | 749.0 | 620.4 | |
| 0.00 | 4.26 | 0.00 | 2.24 | 23.82 | 163.98 | 1.79 | 355.06 | 0.3325 | 833.0 | 653.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 22.98 | 163.80 | 1.61 | 355.32 | 0.3184 | 930.0 | 757.9 | |
| 0.00 | 3.18 | 0.00 | 1.66 | 23.18 | 163.61 | 1.41 | 355.93 | 0.3214 | 946.0 | 756.0 | |
| 0.00 | 2.90 | 0.00 | 1.52 | 23.56 | 163.34 | 1.15 | 356.76 | 0.3275 | 825.0 | 708.9 | |
| 0.00 | 2.27 | 0.00 | 1.18 | 22.95 | 162.41 | 0.22 | 359.36 | 0.3168 | 1011.0 | 726.4 | |
| 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. | |