SDO HMI 2011-07-21 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.27 | 213.14 | 35.30 | 141.04 | 24.70 | 77.82 | -38.09 | 57.60 | 0.6656 | -172.6 | -138.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.24 | 98.54 | 12.40 | 63.51 | 24.09 | 79.66 | -36.25 | 57.50 | 0.6423 | -1038.4 | -435.8 | |
| 1.00 | -1.00 | 0.65 | -1.00 | 24.43 | 79.34 | -36.57 | 57.19 | 0.6478 | -576.8 | 999999 | |
| 3.81 | -1.00 | 2.48 | -1.00 | 24.25 | 79.06 | -36.85 | 57.59 | 0.6499 | -642.1 | 999999 | |
| 3.18 | 4.08 | 2.10 | 2.70 | 25.29 | 78.15 | -37.76 | 56.63 | 0.6653 | -740.5 | -602.9 | |
| 0.00 | 1.27 | 0.00 | 0.83 | 24.39 | 78.47 | -37.44 | 57.72 | 0.6572 | -638.0 | -422.9 | |
| 1.09 | 2.72 | 0.72 | 1.79 | 24.70 | 78.27 | -37.64 | 57.38 | 0.6610 | -604.6 | -579.9 | |
| 1.72 | 6.44 | 1.14 | 4.25 | 24.56 | 78.03 | -37.88 | 57.70 | 0.6630 | -673.4 | -658.1 | |
| 0.00 | 1.36 | 0.00 | 0.89 | 23.16 | 78.51 | -37.40 | 59.45 | 0.6507 | -697.0 | -572.1 | |
| 1.18 | -7.00 | 0.78 | -7.00 | 24.40 | 78.00 | -37.91 | 57.95 | 0.6625 | -732.5 | 999999 | |
| 0.00 | 2.90 | 0.00 | 1.90 | 23.47 | 78.32 | -37.59 | 59.10 | 0.6544 | -253.0 | -405.5 | |
| 0.00 | 1.91 | 0.00 | 1.26 | 25.01 | 77.78 | -38.13 | 57.21 | 0.6679 | -757.0 | -517.8 | |
| 0.00 | 2.18 | 0.00 | 1.44 | 24.61 | 77.63 | -38.28 | 57.85 | 0.6676 | -551.0 | -484.3 | |
| 2.36 | 33.03 | 1.58 | 22.12 | 25.34 | 77.27 | -38.64 | 57.01 | 0.6751 | -633.0 | -180.2 | |
| 0.00 | 1.18 | 0.00 | 0.79 | 24.83 | 77.46 | -38.45 | 57.63 | 0.6705 | -608.0 | -489.0 | |
| 0.00 | 0.91 | 0.00 | 0.62 | 26.54 | 76.79 | -39.12 | 55.63 | 0.6861 | 608.0 | 489.4 | |
| 1.81 | -13.00 | 1.21 | -13.00 | 25.11 | 77.31 | -38.60 | 57.30 | 0.6736 | -760.3 | 999999 | |
| 2.45 | -13.00 | 1.64 | -13.00 | 24.78 | 77.13 | -38.78 | 57.86 | 0.6738 | -575.9 | 999999 | |
| 1.72 | -13.00 | 1.16 | -13.00 | 25.35 | 76.87 | -39.04 | 57.20 | 0.6795 | -277.9 | 999999 | |
| 1.91 | 3.72 | 1.31 | 2.55 | 26.80 | 76.15 | -39.76 | 55.60 | 0.6941 | 740.5 | 642.0 | |
| 0.00 | 2.18 | 0.00 | 1.49 | 26.57 | 76.16 | -39.75 | 55.91 | 0.6929 | 829.0 | 698.2 | |
| 0.00 | 2.63 | 0.00 | 1.76 | 24.63 | 76.88 | -39.03 | 58.18 | 0.6759 | -324.0 | -128.9 | |
| 1.45 | 3.18 | 1.00 | 2.18 | 26.29 | 75.92 | -39.99 | 56.40 | 0.6940 | 775.8 | 578.3 | |
| 0.00 | 1.09 | 0.00 | 0.75 | 26.28 | 75.70 | -40.21 | 56.52 | 0.6963 | 542.0 | 559.8 | |
| 0.00 | 2.90 | 0.00 | 2.03 | 27.10 | 74.90 | -41.01 | 55.82 | 0.7084 | 584.0 | 450.4 | |
| 0.00 | 6.62 | 0.00 | 4.61 | 26.61 | 75.07 | -40.84 | 56.38 | 0.7044 | 774.0 | 604.5 | |
| 4.72 | 16.70 | 3.22 | 11.35 | 24.57 | 75.60 | -40.31 | 58.88 | 0.6895 | 868.6 | 526.1 | |
| 0.00 | 1.45 | 0.00 | 0.98 | 23.92 | 75.71 | -40.19 | 59.72 | 0.6855 | 672.0 | 561.6 | |
| 0.00 | 1.81 | 0.00 | 1.24 | 24.55 | 75.25 | -40.66 | 59.06 | 0.6932 | 656.0 | 570.8 | |
| 0.00 | 0.64 | 0.00 | 0.44 | 24.44 | 75.12 | -40.79 | 59.27 | 0.6942 | 657.0 | 531.9 | |
| 0.00 | 1.45 | 0.00 | 1.02 | 26.03 | 74.05 | -41.86 | 57.62 | 0.7123 | 758.0 | 623.2 | |
| 5.63 | 6.90 | 3.91 | 4.79 | 24.97 | 74.46 | -41.45 | 58.86 | 0.7035 | 769.2 | 595.9 | |
| 0.00 | 1.45 | 0.00 | 1.01 | 24.47 | 74.44 | -41.47 | 59.53 | 0.7017 | 338.0 | 324.4 | |
| 0.00 | 1.36 | 0.00 | 0.96 | 25.66 | 73.85 | -42.06 | 58.20 | 0.7128 | 522.0 | 323.3 | |
| 0.00 | 1.63 | 0.00 | 1.14 | 24.91 | 74.03 | -41.88 | 59.12 | 0.7078 | 665.0 | 497.8 | |
| 0.00 | 0.91 | 0.00 | 0.64 | 25.32 | 73.68 | -42.23 | 58.73 | 0.7132 | 490.0 | 464.8 | |
| 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. | |