SDO HMI 2014-08-01 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.39 | 33.06 | 8.81 | 19.03 | -21.06 | 249.05 | -14.90 | 151.88 | 0.5103 | 669.5 | 435.9 | |
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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 | 0.75 | -17.21 | 251.41 | -12.54 | 151.90 | 0.4423 | -724.0 | -619.7 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -18.21 | 251.17 | -12.78 | 152.54 | 0.4577 | 739.0 | 557.3 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -17.55 | 250.99 | -12.96 | 151.50 | 0.4500 | 714.0 | 586.0 | |
| 0.00 | 2.54 | 0.00 | 1.48 | -23.09 | 250.36 | -13.59 | 155.78 | 0.5289 | 764.0 | 649.6 | |
| 7.24 | 21.28 | 4.15 | 12.18 | -20.58 | 249.14 | -14.82 | 151.51 | 0.5039 | 927.7 | 667.2 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -22.64 | 248.91 | -15.04 | 153.15 | 0.5323 | 788.0 | 636.8 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -22.79 | 248.79 | -15.16 | 153.10 | 0.5349 | 594.0 | 533.5 | |
| 4.53 | -5.00 | 2.59 | -5.00 | -20.35 | 249.02 | -14.93 | 151.09 | 0.5017 | 1124.2 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -23.03 | 248.70 | -15.26 | 153.17 | 0.5387 | 595.0 | 443.1 | |
| 1.99 | -5.00 | 1.14 | -5.00 | -20.59 | 248.90 | -15.06 | 151.13 | 0.5057 | 781.3 | 999999 | |
| 1.63 | -5.00 | 0.93 | -5.00 | -20.42 | 248.85 | -15.11 | 150.88 | 0.5039 | 871.9 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -22.86 | 248.58 | -15.37 | 152.84 | 0.5373 | 703.0 | 565.8 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -20.49 | 248.64 | -15.32 | 150.62 | 0.5064 | 543.0 | 444.7 | |
| 0.00 | 1.18 | 0.00 | 0.77 | -29.66 | 242.76 | -21.19 | 151.31 | 0.6567 | -586.0 | -426.1 | |
| 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. | |