SDO HMI 2014-08-21 18:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.06 | 151.19 | 15.99 | 88.93 | 16.40 | 28.04 | 31.82 | 289.91 | 0.5397 | -738.5 | -338.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.99 | 131.40 | 14.77 | 77.72 | 16.24 | 28.64 | 32.42 | 289.29 | 0.5474 | -1180.5 | -358.7 | |
| 1.44 | -1.00 | 0.85 | -1.00 | 16.33 | 28.25 | 32.02 | 289.60 | 0.5423 | -1160.5 | 999999 | |
| 0.63 | 2.88 | 0.37 | 1.67 | 17.55 | 26.55 | 30.32 | 292.59 | 0.5234 | -859.3 | -672.7 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 16.97 | 26.44 | 30.21 | 291.56 | 0.5196 | -755.0 | -544.1 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 17.48 | 26.09 | 29.87 | 292.70 | 0.5169 | -724.0 | -620.9 | |
| 0.00 | 3.77 | 0.00 | 2.17 | 17.09 | 25.88 | 29.65 | 292.08 | 0.5123 | -994.0 | -829.6 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 17.26 | 25.72 | 29.50 | 292.47 | 0.5108 | -708.0 | -664.6 | |
| 0.00 | 1.26 | 0.00 | 0.72 | 17.27 | 25.54 | 29.32 | 292.58 | 0.5084 | -827.0 | -784.3 | |
| 0.00 | 1.53 | 0.00 | 0.87 | 16.85 | 24.82 | 28.59 | 292.16 | 0.4965 | -835.0 | -693.0 | |
| 0.00 | 2.43 | 0.00 | 1.35 | 18.56 | 21.77 | 25.54 | 297.53 | 0.4628 | 691.0 | 558.4 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 17.55 | 21.47 | 25.24 | 295.69 | 0.4531 | 705.0 | 602.1 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 17.33 | 20.35 | 24.13 | 296.06 | 0.4362 | 809.0 | 661.8 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 18.95 | 20.28 | 24.05 | 299.53 | 0.4449 | 845.0 | 699.8 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 17.18 | 18.85 | 22.62 | 296.99 | 0.4141 | 722.0 | 533.2 | |
| 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. | |