SDO HMI 2014-08-23 13:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.35 | 180.23 | 34.87 | 183.77 | -4.89 | 32.59 | 60.03 | 260.44 | 0.8765 | 200.2 | 242.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.07 | 112.87 | 2.26 | 119.18 | -4.29 | 34.74 | 62.18 | 261.56 | 0.8935 | 286.1 | 513.9 | |
| 0.45 | 2.16 | 0.50 | 2.40 | -6.10 | 34.86 | 62.30 | 259.60 | 0.8969 | 212.0 | 104.3 | |
| 1.71 | -1.00 | 1.87 | -1.00 | -5.29 | 34.58 | 62.01 | 260.43 | 0.8936 | 63.1 | 999999 | |
| 1.35 | 3.32 | 1.48 | 3.64 | -5.69 | 34.52 | 61.95 | 259.98 | 0.8937 | 257.7 | 183.4 | |
| 1.44 | -1.00 | 1.55 | -1.00 | -4.52 | 34.26 | 61.69 | 261.22 | 0.8900 | 619.4 | 999999 | |
| 0.00 | 2.79 | 0.00 | 3.11 | -7.45 | 34.77 | 62.21 | 258.10 | 0.8983 | 503.0 | 354.8 | |
| 4.04 | -1.00 | 4.36 | -1.00 | -5.09 | 34.15 | 61.59 | 260.56 | 0.8900 | 457.0 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.88 | -6.37 | 34.19 | 61.63 | 259.17 | 0.8922 | 379.0 | 351.1 | |
| 2.61 | -1.00 | 2.76 | -1.00 | -4.34 | 33.78 | 61.22 | 261.32 | 0.8860 | 832.4 | 999999 | |
| 1.89 | -1.00 | 2.01 | -1.00 | -4.72 | 33.83 | 61.27 | 260.91 | 0.8869 | 737.2 | 999999 | |
| 11.86 | -1.00 | 12.45 | -1.00 | -4.98 | 33.37 | 60.81 | 260.53 | 0.8836 | 736.8 | 999999 | |
| 0.81 | 2.16 | 0.84 | 2.25 | -5.41 | 33.06 | 60.50 | 259.98 | 0.8818 | 616.9 | 500.5 | |
| 0.00 | 2.43 | 0.00 | 2.51 | -6.35 | 32.61 | 60.05 | 258.83 | 0.8797 | 627.0 | 560.3 | |
| 0.00 | 1.35 | 0.00 | 1.38 | -5.43 | 32.45 | 59.88 | 259.82 | 0.8768 | 629.0 | 572.7 | |
| 0.00 | 0.90 | 0.00 | 0.89 | -3.29 | 31.75 | 59.18 | 262.09 | 0.8676 | -78.0 | -97.7 | |
| 0.00 | 0.63 | 0.00 | 0.62 | -3.63 | 31.72 | 59.16 | 261.71 | 0.8679 | 3.0 | -49.1 | |
| 0.63 | 2.43 | 0.62 | 2.40 | -5.03 | 31.30 | 58.74 | 260.02 | 0.8666 | 634.1 | 591.8 | |
| 0.00 | 1.53 | 0.00 | 1.49 | -4.03 | 31.17 | 58.61 | 261.13 | 0.8638 | -396.0 | -217.5 | |
| 0.00 | 1.62 | 0.00 | 1.54 | -4.08 | 30.19 | 57.63 | 260.86 | 0.8553 | -344.0 | -232.1 | |
| 0.63 | 2.52 | 0.60 | 2.41 | -5.59 | 30.16 | 57.60 | 259.12 | 0.8577 | 684.4 | 638.0 | |
| 0.00 | 0.63 | 0.00 | 0.59 | -4.70 | 29.92 | 57.36 | 260.09 | 0.8540 | -155.0 | -139.9 | |
| 0.00 | 0.54 | 0.00 | 0.51 | -4.38 | 29.83 | 57.26 | 260.44 | 0.8526 | -6.0 | -41.2 | |
| 0.00 | 2.88 | 0.00 | 2.69 | -4.37 | 29.65 | 57.09 | 260.42 | 0.8510 | -491.0 | -300.5 | |
| 0.00 | 1.08 | 0.00 | 1.01 | -5.29 | 29.61 | 57.04 | 259.34 | 0.8522 | 362.0 | 279.0 | |
| 0.00 | 21.39 | 0.00 | 19.84 | -3.93 | 29.33 | 56.76 | 260.85 | 0.8473 | -764.0 | -605.3 | |
| 0.00 | 0.45 | 0.00 | 0.42 | -4.44 | 29.22 | 56.65 | 260.23 | 0.8472 | -370.0 | -332.4 | |
| 0.00 | 0.63 | 0.00 | 0.58 | -4.58 | 29.06 | 56.50 | 260.03 | 0.8461 | -494.0 | -424.7 | |
| 0.00 | 1.08 | 0.00 | 0.99 | -5.06 | 28.90 | 56.34 | 259.44 | 0.8455 | -523.0 | -445.1 | |
| 3.86 | 6.29 | 3.57 | 5.80 | -5.39 | 28.84 | 56.28 | 259.04 | 0.8455 | -607.2 | -441.7 | |
| 0.00 | 1.62 | 0.00 | 1.50 | -5.99 | 28.93 | 56.37 | 258.37 | 0.8475 | -491.0 | -442.7 | |
| 0.00 | 1.08 | 0.00 | 0.99 | -5.39 | 28.51 | 55.95 | 258.96 | 0.8425 | -387.0 | -432.2 | |
| 0.00 | 1.08 | 0.00 | 0.96 | -4.60 | 27.76 | 55.20 | 259.70 | 0.8340 | -519.0 | -414.5 | |
| 0.00 | 0.90 | 0.00 | 0.74 | -6.66 | 24.17 | 51.61 | 256.29 | 0.8035 | -463.0 | -406.3 | |
| 0.00 | 1.17 | 0.00 | 0.96 | -6.43 | 24.09 | 51.53 | 256.54 | 0.8022 | -621.0 | -496.8 | |
| 0.00 | 0.99 | 0.00 | 0.79 | -4.45 | 23.17 | 50.61 | 258.71 | 0.7880 | -542.0 | -463.8 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -6.17 | 21.42 | 48.86 | 256.04 | 0.7738 | -595.0 | -542.4 | |
| 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. | |