SDO HMI 2011-07-17 01:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.72 | 111.11 | 28.80 | 77.68 | -22.82 | 137.32 | -36.45 | 129.14 | 0.7075 | -263.5 | -53.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.45 | 3.99 | 0.30 | 2.65 | -22.89 | 141.57 | -32.20 | 132.44 | 0.6674 | 749.6 | 682.0 | |
| 0.00 | 4.99 | 0.00 | 3.31 | -22.59 | 141.34 | -32.43 | 131.88 | 0.6674 | 799.0 | 748.2 | |
| 0.00 | 3.09 | 0.00 | 2.11 | -25.04 | 140.60 | -33.17 | 134.16 | 0.6933 | 561.0 | 458.4 | |
| 0.00 | 1.00 | 0.00 | 0.69 | -25.32 | 140.51 | -33.26 | 134.41 | 0.6962 | 477.0 | 381.2 | |
| 0.00 | 1.18 | 0.00 | 0.79 | -23.54 | 140.84 | -32.93 | 132.61 | 0.6794 | 606.0 | 571.7 | |
| 4.08 | 6.90 | 2.72 | 4.60 | -22.25 | 140.64 | -33.13 | 130.90 | 0.6715 | 879.9 | 821.0 | |
| 0.00 | 2.09 | 0.00 | 1.39 | -21.85 | 140.39 | -33.38 | 130.22 | 0.6710 | 828.0 | 646.4 | |
| 0.00 | 2.00 | 0.00 | 1.34 | -22.58 | 140.20 | -33.57 | 130.94 | 0.6783 | 657.0 | 513.5 | |
| 0.00 | 1.18 | 0.00 | 0.79 | -22.17 | 140.27 | -33.50 | 130.50 | 0.6745 | 518.0 | 437.0 | |
| 0.00 | 0.91 | 0.00 | 0.61 | -22.82 | 140.01 | -33.76 | 131.09 | 0.6819 | 470.0 | 309.4 | |
| 1.09 | 3.81 | 0.73 | 2.57 | -22.45 | 139.95 | -33.82 | 130.60 | 0.6797 | 459.7 | 427.7 | |
| 0.00 | 1.27 | 0.00 | 0.84 | -20.83 | 140.03 | -33.74 | 128.66 | 0.6671 | 586.0 | 529.6 | |
| 0.00 | 0.64 | 0.00 | 0.43 | -23.13 | 139.32 | -34.45 | 130.92 | 0.6908 | 260.0 | 292.1 | |
| 0.00 | 3.18 | 0.00 | 2.16 | -21.80 | 138.70 | -35.07 | 128.85 | 0.6873 | 615.0 | 420.6 | |
| 0.00 | 1.00 | 0.00 | 0.69 | -22.36 | 138.29 | -35.48 | 129.23 | 0.6952 | 642.0 | 471.3 | |
| 0.00 | 1.09 | 0.00 | 0.75 | -22.23 | 138.13 | -35.64 | 128.96 | 0.6959 | 611.0 | 504.4 | |
| 0.00 | 1.09 | 0.00 | 0.75 | -22.07 | 138.06 | -35.71 | 128.70 | 0.6955 | 398.0 | 354.5 | |
| 0.00 | 2.09 | 0.00 | 1.44 | -22.15 | 137.71 | -36.06 | 128.55 | 0.6995 | -228.0 | -204.4 | |
| 15.88 | 43.66 | 11.16 | 30.73 | -22.47 | 136.70 | -37.07 | 128.23 | 0.7114 | -941.8 | -676.1 | |
| 2.36 | -19.00 | 1.67 | -19.00 | -22.73 | 136.29 | -37.48 | 128.25 | 0.7170 | -706.5 | 999999 | |
| 1.72 | -19.00 | 1.22 | -19.00 | -22.46 | 136.29 | -37.48 | 127.93 | 0.7152 | -761.3 | 999999 | |
| 2.81 | -19.00 | 2.00 | -19.00 | -22.72 | 135.92 | -37.85 | 127.98 | 0.7205 | -637.0 | 999999 | |
| 6.53 | 7.62 | 4.71 | 5.49 | -23.12 | 135.40 | -38.37 | 128.12 | 0.7279 | -772.6 | -635.8 | |
| 0.00 | 2.72 | 0.00 | 2.00 | -24.28 | 134.82 | -38.95 | 129.09 | 0.7406 | -741.0 | -623.0 | |
| 0.00 | 0.91 | 0.00 | 0.66 | -23.32 | 134.73 | -39.04 | 127.92 | 0.7354 | -603.0 | -473.0 | |
| 0.00 | 1.00 | 0.00 | 0.73 | -23.82 | 134.38 | -39.39 | 128.27 | 0.7417 | -727.0 | -655.5 | |
| 0.00 | 1.36 | 0.00 | 1.01 | -23.90 | 134.14 | -39.63 | 128.21 | 0.7445 | -618.0 | -546.0 | |
| 4.08 | 4.18 | 3.00 | 3.07 | -23.45 | 134.21 | -39.56 | 127.74 | 0.7410 | -777.8 | -776.0 | |
| 0.00 | 1.00 | 0.00 | 0.75 | -24.61 | 133.78 | -39.99 | 128.80 | 0.7520 | -460.0 | -298.5 | |
| 0.00 | 1.27 | 0.00 | 0.94 | -23.85 | 133.85 | -39.92 | 127.97 | 0.7468 | -433.0 | -314.1 | |
| 0.00 | 1.27 | 0.00 | 0.93 | -22.78 | 134.11 | -39.66 | 126.88 | 0.7380 | -571.0 | -457.6 | |
| 0.00 | 1.45 | 0.00 | 1.08 | -23.58 | 133.73 | -40.04 | 127.59 | 0.7462 | -624.0 | -509.2 | |
| 0.00 | 0.45 | 0.00 | 0.34 | -23.87 | 133.45 | -40.32 | 127.74 | 0.7506 | -345.0 | -357.6 | |
| 1.72 | 2.72 | 1.29 | 2.04 | -23.82 | 133.12 | -40.65 | 127.48 | 0.7533 | -537.9 | -407.0 | |
| 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. | |