SDO HMI 2014-08-06 02:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.06 | 114.75 | 27.28 | 85.82 | -8.21 | 249.73 | 46.41 | 253.27 | 0.7504 | 153.3 | 53.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 1.12 | -6.57 | 254.93 | 51.61 | 257.01 | 0.8013 | 312.0 | 329.5 | |
| 0.00 | 1.18 | 0.00 | 0.97 | -6.81 | 254.81 | 51.50 | 256.69 | 0.8007 | 645.0 | 531.6 | |
| 0.00 | 0.72 | 0.00 | 0.59 | -7.77 | 254.47 | 51.16 | 255.41 | 0.7996 | 467.0 | 407.2 | |
| 0.00 | 0.63 | 0.00 | 0.52 | -7.98 | 254.31 | 51.00 | 255.12 | 0.7985 | 440.0 | 375.3 | |
| 6.51 | 8.95 | 5.25 | 7.22 | -6.76 | 253.93 | 50.61 | 256.49 | 0.7915 | 637.5 | 389.0 | |
| 0.00 | 1.36 | 0.00 | 1.08 | -5.76 | 253.50 | 50.19 | 257.61 | 0.7847 | -310.0 | -295.3 | |
| 1.08 | 4.43 | 0.86 | 3.52 | -7.31 | 253.09 | 49.77 | 255.56 | 0.7842 | 537.4 | 396.7 | |
| 0.00 | 1.08 | 0.00 | 0.85 | -7.07 | 252.44 | 49.12 | 255.67 | 0.7767 | 433.0 | 397.3 | |
| 0.00 | 0.99 | 0.00 | 0.77 | -5.16 | 252.21 | 48.89 | 258.01 | 0.7694 | 539.0 | 465.5 | |
| 0.00 | 1.45 | 0.00 | 1.13 | -7.30 | 252.14 | 48.83 | 255.29 | 0.7742 | 382.0 | 352.4 | |
| 1.27 | 2.44 | 0.97 | 1.87 | -6.31 | 251.50 | 48.18 | 256.34 | 0.7646 | 603.8 | 516.7 | |
| 0.54 | 2.80 | 0.41 | 2.14 | -6.51 | 251.34 | 48.02 | 256.03 | 0.7634 | 750.8 | 600.9 | |
| 0.00 | 1.18 | 0.00 | 0.89 | -8.31 | 250.41 | 47.09 | 253.43 | 0.7584 | 558.0 | 464.8 | |
| 0.00 | 0.99 | 0.00 | 0.75 | -8.47 | 250.12 | 46.80 | 253.12 | 0.7558 | 528.0 | 513.5 | |
| 5.06 | 7.32 | 3.76 | 5.44 | -8.02 | 249.51 | 46.19 | 253.49 | 0.7476 | 615.5 | 373.1 | |
| 7.41 | 14.83 | 5.46 | 10.92 | -6.79 | 249.35 | 46.03 | 255.03 | 0.7420 | 756.0 | 566.2 | |
| 0.00 | 2.44 | 0.00 | 1.80 | -7.25 | 249.23 | 45.91 | 254.39 | 0.7421 | 726.0 | 587.4 | |
| 0.81 | -16.00 | 0.60 | -16.00 | -6.96 | 249.10 | 45.78 | 254.72 | 0.7398 | 881.7 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.96 | -10.92 | 249.70 | 46.39 | 249.86 | 0.7595 | -646.0 | -454.1 | |
| 4.52 | 39.15 | 3.38 | 29.14 | -9.61 | 249.41 | 46.09 | 251.41 | 0.7517 | -566.4 | -303.1 | |
| 0.36 | 1.45 | 0.27 | 1.06 | -7.29 | 249.01 | 45.69 | 254.25 | 0.7398 | 618.8 | 509.7 | |
| 6.33 | -20.00 | 4.71 | -20.00 | -9.68 | 249.16 | 45.84 | 251.21 | 0.7492 | -777.9 | 999999 | |
| 2.17 | -20.00 | 1.61 | -20.00 | -9.63 | 248.88 | 45.56 | 251.17 | 0.7460 | -783.1 | 999999 | |
| 0.00 | 2.26 | 0.00 | 1.68 | -10.19 | 248.80 | 45.49 | 250.43 | 0.7472 | -550.0 | -445.8 | |
| 0.00 | 1.18 | 0.00 | 0.85 | -7.33 | 247.92 | 44.61 | 253.81 | 0.7276 | 427.0 | 429.8 | |
| 0.00 | 1.27 | 0.00 | 0.91 | -7.11 | 247.85 | 44.54 | 254.08 | 0.7260 | 582.0 | 540.1 | |
| 0.00 | 1.18 | 0.00 | 0.83 | -3.80 | 247.50 | 44.19 | 258.44 | 0.7121 | 571.0 | 361.1 | |
| 0.00 | 1.72 | 0.00 | 1.22 | -8.17 | 247.05 | 43.73 | 252.36 | 0.7203 | 664.0 | 590.5 | |
| 0.00 | 2.17 | 0.00 | 1.55 | -10.94 | 246.29 | 42.98 | 248.37 | 0.7223 | -80.0 | -91.5 | |
| 0.00 | 1.18 | 0.00 | 0.85 | -12.33 | 246.56 | 43.24 | 246.70 | 0.7310 | -399.0 | -342.2 | |
| 0.00 | 1.36 | 0.00 | 0.96 | -11.21 | 245.71 | 42.39 | 247.74 | 0.7169 | -487.0 | -330.4 | |
| 0.00 | 2.17 | 0.00 | 1.48 | -9.96 | 243.64 | 40.32 | 248.42 | 0.6877 | -498.0 | -394.1 | |
| 0.00 | 1.72 | 0.00 | 1.12 | -7.07 | 241.81 | 38.49 | 251.62 | 0.6532 | -509.0 | -452.5 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -7.39 | 241.57 | 38.25 | 251.02 | 0.6515 | -671.0 | -534.6 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -2.24 | 240.92 | 37.60 | 258.55 | 0.6243 | -580.0 | -479.2 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -7.57 | 240.46 | 37.14 | 250.21 | 0.6383 | -596.0 | -613.3 | |
| 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. | |