SDO HMI 2011-11-25 16:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.03 | 67.08 | 20.04 | 37.25 | 17.79 | 214.12 | -21.86 | 51.58 | 0.4541 | 408.1 | 138.0 | |
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back to the solar disc SDO HMI 2011-11-25 16:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.20 | 0.00 | 0.65 | 18.48 | 217.35 | -18.62 | 46.08 | 0.4222 | 816.0 | 558.1 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 18.54 | 217.25 | -18.73 | 46.13 | 0.4240 | 813.0 | 649.7 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 19.22 | 216.34 | -19.63 | 46.23 | 0.4413 | 402.0 | 575.0 | |
| 7.70 | 12.66 | 4.22 | 6.94 | 17.24 | 215.81 | -20.16 | 50.54 | 0.4282 | -985.9 | -786.3 | |
| 0.00 | 2.65 | 0.00 | 1.47 | 19.30 | 215.53 | -20.45 | 47.18 | 0.4514 | 577.0 | 691.7 | |
| 1.03 | -4.00 | 0.56 | -4.00 | 17.26 | 215.55 | -20.43 | 50.84 | 0.4317 | -845.7 | 999999 | |
| 1.11 | -4.00 | 0.61 | -4.00 | 17.23 | 215.45 | -20.52 | 51.02 | 0.4326 | -819.6 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.13 | 17.17 | 215.16 | -20.81 | 51.51 | 0.4356 | -760.0 | -559.1 | |
| 1.80 | 10.44 | 0.99 | 5.77 | 17.91 | 214.90 | -21.07 | 50.47 | 0.4454 | -809.6 | -605.1 | |
| 0.00 | 2.65 | 0.00 | 1.48 | 17.98 | 213.45 | -22.52 | 52.07 | 0.4638 | 902.0 | 733.2 | |
| 2.40 | 33.03 | 1.34 | 18.49 | 17.52 | 213.21 | -22.76 | 53.19 | 0.4628 | 955.5 | 810.7 | |
| 21.99 | -11.00 | 12.32 | -11.00 | 17.82 | 212.90 | -23.07 | 52.98 | 0.4692 | 1010.7 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 18.13 | 212.59 | -23.39 | 52.79 | 0.4756 | 488.0 | 407.3 | |
| 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. | |