SDO HMI 2014-08-05 18:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.80 | 103.44 | 23.86 | 71.85 | -7.73 | 250.00 | 42.27 | 252.32 | 0.7012 | 299.1 | 242.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 1.42 | -6.54 | 254.66 | 46.92 | 255.68 | 0.7512 | 782.0 | 673.5 | |
| 0.00 | 0.90 | 0.00 | 0.68 | -7.82 | 254.25 | 46.51 | 253.89 | 0.7504 | 491.0 | 416.2 | |
| 0.00 | 1.27 | 0.00 | 0.94 | -7.90 | 254.03 | 46.30 | 253.72 | 0.7483 | 363.0 | 367.1 | |
| 8.95 | 11.21 | 6.56 | 8.22 | -6.80 | 253.53 | 45.79 | 254.97 | 0.7393 | 743.5 | 457.1 | |
| 0.00 | 0.72 | 0.00 | 0.52 | -6.31 | 252.91 | 45.17 | 255.40 | 0.7307 | -531.0 | -469.4 | |
| 3.89 | 5.69 | 2.83 | 4.14 | -7.35 | 252.99 | 45.25 | 254.06 | 0.7348 | 625.8 | 457.9 | |
| 1.08 | 4.61 | 0.78 | 3.32 | -7.18 | 252.40 | 44.66 | 254.07 | 0.7276 | 559.8 | 414.3 | |
| 0.00 | 1.45 | 0.00 | 1.03 | -7.36 | 251.90 | 44.17 | 253.65 | 0.7224 | 635.0 | 527.7 | |
| 1.45 | 7.41 | 1.02 | 5.20 | -6.37 | 251.24 | 43.50 | 254.73 | 0.7114 | 688.3 | 590.7 | |
| 1.17 | -9.00 | 0.82 | -9.00 | -6.45 | 251.08 | 43.34 | 254.56 | 0.7098 | 839.6 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.94 | -6.45 | 250.66 | 42.92 | 254.40 | 0.7048 | 835.0 | 708.8 | |
| 0.00 | 1.17 | 0.00 | 0.82 | -6.53 | 250.41 | 42.67 | 254.21 | 0.7022 | 470.0 | 476.6 | |
| 0.00 | 0.63 | 0.00 | 0.44 | -7.86 | 250.32 | 42.58 | 252.34 | 0.7057 | 598.0 | 582.0 | |
| 0.00 | 0.63 | 0.00 | 0.44 | -6.59 | 249.96 | 42.22 | 253.95 | 0.6970 | 525.0 | 399.9 | |
| 0.00 | 2.35 | 0.00 | 1.63 | -8.63 | 249.71 | 41.97 | 251.04 | 0.7014 | 642.0 | 507.3 | |
| 0.00 | 0.72 | 0.00 | 0.51 | -11.02 | 250.08 | 42.34 | 248.01 | 0.7153 | -354.0 | -339.9 | |
| 4.25 | 13.10 | 2.90 | 8.94 | -6.85 | 249.24 | 41.51 | 253.30 | 0.6892 | 894.5 | 660.1 | |
| 2.53 | 6.05 | 1.74 | 4.16 | -7.94 | 249.29 | 41.55 | 251.80 | 0.6938 | 806.3 | 623.4 | |
| 2.71 | 23.04 | 1.88 | 15.86 | -9.36 | 249.40 | 41.66 | 249.91 | 0.7006 | -452.0 | -391.2 | |
| 0.54 | -17.00 | 0.37 | -17.00 | -7.02 | 249.02 | 41.28 | 252.97 | 0.6871 | 923.5 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.76 | -10.95 | 249.57 | 41.83 | 247.86 | 0.7092 | -571.0 | -445.9 | |
| 0.00 | 0.99 | 0.00 | 0.69 | -10.59 | 249.47 | 41.73 | 248.28 | 0.7065 | -542.0 | -436.5 | |
| 0.00 | 0.54 | 0.00 | 0.37 | -7.20 | 248.96 | 41.22 | 252.69 | 0.6870 | 665.0 | 628.7 | |
| 0.00 | 1.81 | 0.00 | 1.22 | -6.66 | 248.82 | 41.08 | 253.39 | 0.6834 | 87.0 | 126.0 | |
| 0.00 | 0.63 | 0.00 | 0.43 | -8.22 | 248.87 | 41.13 | 251.23 | 0.6899 | 524.0 | 461.0 | |
| 3.80 | -19.00 | 2.61 | -19.00 | -9.39 | 248.99 | 41.25 | 249.68 | 0.6960 | -712.8 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.43 | -7.92 | 248.59 | 40.85 | 251.52 | 0.6854 | 531.0 | 481.9 | |
| 3.43 | -19.00 | 2.35 | -19.00 | -9.30 | 248.65 | 40.91 | 249.64 | 0.6916 | -886.5 | 999999 | |
| 0.00 | 2.44 | 0.00 | 1.63 | -7.19 | 247.94 | 40.20 | 252.27 | 0.6746 | 844.0 | 652.7 | |
| 0.00 | 1.36 | 0.00 | 0.91 | -7.64 | 247.75 | 40.01 | 251.54 | 0.6741 | 789.0 | 688.8 | |
| 0.00 | 2.80 | 0.00 | 1.86 | -8.15 | 247.01 | 39.27 | 250.47 | 0.6671 | 830.0 | 666.0 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -6.17 | 246.73 | 38.99 | 253.20 | 0.6557 | 631.0 | 504.5 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -9.83 | 245.36 | 37.63 | 247.23 | 0.6547 | -381.0 | -325.9 | |
| 0.00 | 2.17 | 0.00 | 1.33 | -6.98 | 241.46 | 33.72 | 249.29 | 0.5913 | -703.0 | -625.0 | |
| 0.00 | 1.17 | 0.00 | 0.72 | -7.19 | 241.33 | 33.59 | 248.88 | 0.5906 | -428.0 | -438.8 | |
| 0.00 | 1.72 | 0.00 | 1.05 | -7.00 | 241.27 | 33.54 | 249.15 | 0.5890 | -763.0 | -546.6 | |
| 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. | |