SDO HMI 2014-08-13 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.20 | 373.70 | 37.48 | 214.31 | 15.13 | 133.72 | 29.54 | 288.93 | 0.5050 | -850.1 | -330.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.89 | 357.67 | 1.10 | 205.68 | 15.74 | 134.48 | 30.30 | 289.78 | 0.5182 | -867.0 | -370.7 | |
| 62.86 | -1.00 | 36.14 | -1.00 | 15.24 | 134.00 | 29.82 | 289.05 | 0.5096 | -1347.8 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 18.46 | 129.35 | 25.17 | 298.23 | 0.4599 | -871.0 | -714.0 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 11.00 | 127.52 | 23.34 | 282.58 | 0.4002 | 303.0 | 406.0 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 11.74 | 127.32 | 23.14 | 284.50 | 0.3991 | -786.0 | -615.6 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 12.99 | 127.44 | 23.26 | 287.49 | 0.4051 | 533.0 | 455.9 | |
| 0.00 | 1.62 | 0.00 | 0.88 | 12.78 | 127.38 | 23.20 | 287.01 | 0.4035 | 691.0 | 580.3 | |
| 0.00 | 0.63 | 0.00 | 0.34 | 10.28 | 127.13 | 22.95 | 280.93 | 0.3924 | 584.0 | 389.7 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 12.63 | 127.30 | 23.12 | 286.69 | 0.4017 | 814.0 | 624.1 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 12.45 | 127.11 | 22.93 | 286.36 | 0.3983 | 970.0 | 824.1 | |
| 0.00 | 1.62 | 0.00 | 0.88 | 12.73 | 127.00 | 22.83 | 287.11 | 0.3976 | 771.0 | 706.7 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 12.23 | 126.52 | 22.34 | 286.14 | 0.3884 | 772.0 | 627.5 | |
| 0.45 | 2.98 | 0.24 | 1.59 | 10.53 | 125.71 | 21.53 | 282.09 | 0.3706 | 958.8 | 748.8 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 10.61 | 125.15 | 20.97 | 282.55 | 0.3620 | 762.0 | 568.9 | |
| 0.00 | 1.44 | 0.00 | 0.76 | 10.31 | 124.37 | 20.19 | 282.06 | 0.3488 | 1017.0 | 931.1 | |
| 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. | |