SDO HMI 2011-07-23 02:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.83 | 111.40 | 25.63 | 83.58 | -23.06 | 134.43 | 40.59 | 232.90 | 0.7520 | -245.4 | -101.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.73 | 0.00 | 0.62 | -22.55 | 142.35 | 48.52 | 237.80 | 0.8198 | 375.0 | 308.0 | |
| 0.00 | 1.09 | 0.00 | 0.92 | -23.38 | 141.11 | 47.27 | 236.28 | 0.8129 | 423.0 | 348.9 | |
| 0.00 | 2.54 | 0.00 | 2.09 | -23.22 | 139.68 | 45.84 | 235.75 | 0.7999 | 615.0 | 482.0 | |
| 0.00 | 1.09 | 0.00 | 0.88 | -22.32 | 139.05 | 45.22 | 236.44 | 0.7902 | 621.0 | 559.9 | |
| 0.00 | 0.82 | 0.00 | 0.67 | -23.23 | 139.35 | 45.51 | 235.56 | 0.7971 | 552.0 | 525.3 | |
| 0.00 | 1.36 | 0.00 | 1.13 | -24.31 | 139.45 | 45.62 | 234.42 | 0.8031 | 622.0 | 509.3 | |
| 0.00 | 1.72 | 0.00 | 1.38 | -22.81 | 138.70 | 44.86 | 235.69 | 0.7894 | 598.0 | 513.9 | |
| 0.00 | 0.91 | 0.00 | 0.73 | -23.12 | 138.73 | 44.90 | 235.36 | 0.7912 | 458.0 | 406.5 | |
| 0.00 | 1.09 | 0.00 | 0.89 | -24.38 | 139.06 | 45.22 | 234.12 | 0.8001 | 630.0 | 542.8 | |
| 0.00 | 0.27 | 0.00 | 0.22 | -23.39 | 138.57 | 44.73 | 234.98 | 0.7910 | 437.0 | 374.7 | |
| 0.00 | 1.18 | 0.00 | 0.95 | -23.10 | 138.40 | 44.56 | 235.21 | 0.7882 | 505.0 | 511.0 | |
| 2.00 | 7.98 | 1.59 | 6.37 | -22.84 | 138.15 | 44.32 | 235.37 | 0.7847 | 875.5 | 676.4 | |
| 0.00 | 0.63 | 0.00 | 0.52 | -23.97 | 138.59 | 44.75 | 234.33 | 0.7941 | 519.0 | 449.6 | |
| 0.00 | 0.73 | 0.00 | 0.57 | -22.85 | 137.74 | 43.90 | 235.13 | 0.7811 | 643.0 | 589.1 | |
| 0.00 | 1.00 | 0.00 | 0.78 | -22.51 | 137.23 | 43.40 | 235.25 | 0.7748 | 788.0 | 646.0 | |
| 0.00 | 2.36 | 0.00 | 1.84 | -22.68 | 137.26 | 43.42 | 235.06 | 0.7759 | 777.0 | 701.6 | |
| 0.00 | 0.73 | 0.00 | 0.55 | -22.95 | 134.98 | 41.15 | 233.44 | 0.7567 | -308.0 | -273.8 | |
| 0.00 | 2.81 | 0.00 | 2.11 | -22.78 | 134.87 | 41.04 | 233.57 | 0.7547 | -456.0 | -387.2 | |
| 0.00 | 1.18 | 0.00 | 0.88 | -22.82 | 134.54 | 40.71 | 233.32 | 0.7519 | -574.0 | -416.4 | |
| 0.00 | 0.54 | 0.00 | 0.40 | -21.47 | 134.02 | 40.19 | 234.59 | 0.7392 | -473.0 | -430.5 | |
| 0.00 | 3.08 | 0.00 | 2.29 | -22.59 | 134.15 | 40.32 | 233.34 | 0.7470 | -633.0 | -423.6 | |
| 2.90 | 3.27 | 2.14 | 2.41 | -22.24 | 133.90 | 40.07 | 233.60 | 0.7425 | -613.4 | -624.8 | |
| 0.00 | 1.18 | 0.00 | 0.88 | -23.06 | 133.84 | 40.01 | 232.61 | 0.7468 | -69.0 | -55.5 | |
| 3.36 | 46.80 | 2.49 | 34.47 | -23.28 | 133.58 | 39.74 | 232.19 | 0.7457 | -433.3 | -328.1 | |
| 3.99 | -24.00 | 2.93 | -24.00 | -22.79 | 133.36 | 39.52 | 232.62 | 0.7407 | -683.3 | 999999 | |
| 7.44 | -24.00 | 5.48 | -24.00 | -23.19 | 133.24 | 39.41 | 232.07 | 0.7421 | -731.9 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.01 | -23.89 | 133.50 | 39.66 | 231.43 | 0.7487 | -375.0 | -279.0 | |
| 6.80 | -24.00 | 4.98 | -24.00 | -23.21 | 132.90 | 39.07 | 231.84 | 0.7390 | -790.1 | 999999 | |
| 0.00 | 3.08 | 0.00 | 2.25 | -23.32 | 132.56 | 38.73 | 231.48 | 0.7366 | -670.0 | -633.4 | |
| 1.63 | 4.54 | 1.18 | 3.29 | -22.97 | 132.40 | 38.56 | 231.78 | 0.7329 | -657.8 | -662.3 | |
| 0.00 | 1.63 | 0.00 | 1.20 | -23.57 | 132.60 | 38.77 | 231.22 | 0.7385 | -347.0 | -302.7 | |
| 5.44 | 9.80 | 3.92 | 7.06 | -22.75 | 132.07 | 38.23 | 231.82 | 0.7284 | -894.6 | -728.1 | |
| 1.27 | 2.09 | 0.92 | 1.51 | -23.86 | 131.68 | 37.85 | 230.27 | 0.7320 | -708.9 | -623.2 | |
| 0.00 | 1.45 | 0.00 | 1.02 | -21.96 | 130.90 | 37.07 | 231.94 | 0.7122 | -766.0 | -599.2 | |
| 0.00 | 2.36 | 0.00 | 1.69 | -24.42 | 130.66 | 36.82 | 228.91 | 0.7264 | -677.0 | -554.2 | |
| 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. | |