SDO HMI 2011-07-18 15:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.20 | 255.49 | 16.97 | 134.65 | 16.70 | 168.90 | 16.06 | 308.77 | 0.3417 | -691.8 | -374.5 | |
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back to the solar disc SDO HMI 2011-07-18 15:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.50 | 244.78 | 10.82 | 129.06 | 16.60 | 169.26 | 16.42 | 307.89 | 0.3446 | -1342.5 | -421.2 | |
| 1.09 | -1.00 | 0.57 | -1.00 | 17.01 | 169.16 | 16.32 | 309.01 | 0.3473 | -791.3 | 999999 | |
| 6.80 | -1.00 | 3.58 | -1.00 | 16.33 | 169.00 | 16.16 | 307.63 | 0.3387 | -1463.1 | 999999 | |
| 1.54 | -1.00 | 0.81 | -1.00 | 16.89 | 168.99 | 16.14 | 309.01 | 0.3439 | -990.6 | 999999 | |
| 2.27 | -1.00 | 1.19 | -1.00 | 16.61 | 168.73 | 15.89 | 308.78 | 0.3379 | -1340.5 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 15.94 | 166.74 | 13.90 | 310.68 | 0.3058 | -870.0 | -584.3 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 19.26 | 164.55 | 11.71 | 323.00 | 0.3198 | 676.0 | 580.8 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 22.92 | 164.21 | 11.37 | 330.08 | 0.3655 | 830.0 | 611.1 | |
| 0.00 | 2.00 | 0.00 | 1.03 | 17.81 | 162.79 | 9.95 | 324.35 | 0.2835 | 916.0 | 686.8 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 17.59 | 162.68 | 9.84 | 324.17 | 0.2795 | 888.0 | 725.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 23.17 | 162.78 | 9.94 | 333.57 | 0.3580 | 854.0 | 726.0 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 21.61 | 161.71 | 8.86 | 333.96 | 0.3277 | 857.0 | 660.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 20.42 | 160.26 | 7.41 | 336.10 | 0.2998 | 1187.0 | 985.4 | |
| 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. | |