SDO HMI 2014-08-20 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.56 | 92.80 | 17.87 | 64.58 | -9.48 | 332.26 | -41.60 | 111.08 | 0.7036 | 681.7 | 345.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.65 | -11.62 | 344.09 | -29.77 | 121.81 | 0.5744 | 599.0 | 464.2 | |
| 0.00 | 1.71 | 0.00 | 1.10 | -10.35 | 337.87 | -35.99 | 115.32 | 0.6417 | 702.0 | 577.9 | |
| 0.00 | 1.17 | 0.00 | 0.75 | -9.05 | 337.96 | -35.90 | 113.50 | 0.6336 | 707.0 | 623.8 | |
| 0.00 | 1.26 | 0.00 | 0.82 | -10.55 | 337.69 | -36.17 | 115.49 | 0.6450 | 554.0 | 518.7 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -9.41 | 336.84 | -37.01 | 113.36 | 0.6492 | 666.0 | 496.0 | |
| 0.00 | 1.08 | 0.00 | 0.75 | -13.13 | 333.49 | -40.36 | 116.49 | 0.7070 | -600.0 | -482.0 | |
| 11.52 | 72.28 | 7.99 | 50.23 | -9.35 | 332.35 | -41.51 | 110.89 | 0.7022 | 1046.8 | 344.5 | |
| 9.00 | -7.00 | 6.27 | -7.00 | -9.58 | 332.23 | -41.63 | 111.14 | 0.7046 | 728.1 | 999999 | |
| 4.41 | 6.39 | 3.15 | 4.57 | -9.31 | 330.47 | -43.39 | 109.98 | 0.7235 | 733.8 | 541.2 | |
| 0.63 | 1.98 | 0.46 | 1.43 | -9.40 | 329.86 | -44.00 | 109.82 | 0.7307 | 555.7 | 458.3 | |
| 0.00 | 1.44 | 0.00 | 1.03 | -7.18 | 329.79 | -44.06 | 106.87 | 0.7233 | 592.0 | 499.2 | |
| 0.00 | 0.99 | 0.00 | 0.72 | -8.05 | 329.12 | -44.74 | 107.75 | 0.7341 | 581.0 | 516.0 | |
| 0.00 | 1.35 | 0.00 | 0.99 | -9.42 | 328.86 | -45.00 | 109.42 | 0.7419 | 443.0 | 377.8 | |
| 0.00 | 1.17 | 0.00 | 0.96 | -9.73 | 323.67 | -50.19 | 107.81 | 0.7974 | -615.0 | -488.5 | |
| 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. | |