| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.41 | 164.08 | 27.18 | 235.42 | 9.17 | 56.52 | -69.92 | 81.63 | 0.9384 | -485.1 | -96.5 | |
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back to the solar disc SDO HMI 2011-11-06 16:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.27 | 159.94 | 21.22 | 226.33 | 9.12 | 56.99 | -69.45 | 81.69 | 0.9359 | -649.4 | -92.8 | |
| 2.07 | -1.00 | 2.97 | -1.00 | 9.35 | 56.27 | -70.17 | 81.44 | 0.9402 | -87.9 | 999999 | |
| 2.07 | -1.00 | 2.99 | -1.00 | 9.19 | 56.16 | -70.28 | 81.61 | 0.9408 | 136.9 | 999999 | |
| 0.00 | 1.12 | 0.00 | 2.42 | 10.29 | 49.26 | -77.19 | 80.32 | 0.9743 | -234.0 | -261.0 | |
| 0.00 | 3.02 | 0.00 | 6.67 | 9.48 | 48.91 | -77.53 | 81.14 | 0.9757 | -289.0 | -149.1 | |
| 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. | |