SDO HMI 2011-07-18 20:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.48 | 242.36 | 18.45 | 129.64 | 16.98 | 168.64 | 18.57 | 305.66 | 0.3777 | -552.5 | -334.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.91 | 223.23 | 0.49 | 119.48 | 16.52 | 169.62 | 19.56 | 303.23 | 0.3853 | -583.8 | -433.3 | |
| 26.40 | -1.00 | 14.13 | -1.00 | 16.65 | 169.13 | 19.06 | 304.16 | 0.3798 | -1294.7 | 999999 | |
| 6.17 | -1.00 | 3.30 | -1.00 | 16.35 | 169.03 | 18.97 | 303.58 | 0.3759 | -1430.5 | 999999 | |
| 1.00 | -1.00 | 0.53 | -1.00 | 17.00 | 168.93 | 18.87 | 305.21 | 0.3800 | -809.0 | 999999 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 20.65 | 166.29 | 16.22 | 316.85 | 0.3838 | 742.0 | 638.0 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 23.10 | 165.37 | 15.30 | 322.74 | 0.4027 | 726.0 | 557.4 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 18.98 | 164.48 | 14.41 | 316.74 | 0.3448 | 828.0 | 650.3 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 23.05 | 164.44 | 14.37 | 324.32 | 0.3933 | 827.0 | 672.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 17.60 | 162.72 | 12.65 | 317.29 | 0.3091 | 973.0 | 661.4 | |
| 0.00 | 1.72 | 0.00 | 0.93 | 23.53 | 163.13 | 13.06 | 327.53 | 0.3875 | 716.0 | 528.8 | |
| 0.00 | 2.63 | 0.00 | 1.41 | 23.28 | 162.76 | 12.69 | 327.86 | 0.3811 | 787.0 | 576.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 21.53 | 162.03 | 11.96 | 326.57 | 0.3515 | 694.0 | 536.9 | |
| 0.00 | 2.09 | 0.00 | 1.10 | 22.12 | 161.17 | 11.10 | 329.39 | 0.3520 | 806.0 | 715.7 | |
| 0.00 | 4.35 | 0.00 | 2.28 | 20.44 | 160.48 | 10.41 | 328.22 | 0.3231 | 943.0 | 756.2 | |
| 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. | |