SDO HMI 2014-08-13 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.64 | 382.60 | 36.92 | 224.76 | 14.95 | 133.33 | 31.92 | 287.58 | 0.5379 | -906.5 | -284.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.85 | 345.40 | 35.41 | 204.31 | 15.30 | 134.00 | 32.59 | 288.05 | 0.5486 | -1387.3 | -378.9 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 14.29 | 132.46 | 31.05 | 286.73 | 0.5240 | -728.0 | -583.1 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 16.54 | 131.96 | 30.55 | 291.15 | 0.5244 | -601.0 | -542.5 | |
| 0.00 | 1.71 | 0.00 | 0.95 | 10.93 | 127.68 | 26.27 | 281.42 | 0.4451 | 747.0 | 652.4 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 12.01 | 127.54 | 26.13 | 283.86 | 0.4456 | -646.0 | -579.3 | |
| 0.00 | 3.24 | 0.00 | 1.79 | 12.75 | 127.49 | 26.08 | 285.52 | 0.4468 | 510.0 | 564.4 | |
| 0.00 | 1.53 | 0.00 | 0.85 | 12.29 | 127.44 | 26.03 | 284.53 | 0.4447 | 655.0 | 473.0 | |
| 0.00 | 2.88 | 0.00 | 1.59 | 12.45 | 127.25 | 25.84 | 284.97 | 0.4423 | 884.0 | 762.2 | |
| 0.00 | 4.33 | 0.00 | 2.39 | 12.91 | 127.19 | 25.78 | 286.02 | 0.4429 | 674.0 | 639.4 | |
| 0.00 | 2.25 | 0.00 | 1.23 | 12.11 | 126.18 | 24.77 | 284.63 | 0.4251 | 933.0 | 743.4 | |
| 1.35 | 14.15 | 0.73 | 7.69 | 10.24 | 125.67 | 24.26 | 280.38 | 0.4127 | 957.8 | 671.2 | |
| 0.00 | 2.70 | 0.00 | 1.47 | 9.60 | 125.55 | 24.14 | 278.87 | 0.4098 | 684.0 | 749.4 | |
| 1.44 | -11.00 | 0.78 | -11.00 | 10.25 | 125.50 | 24.09 | 280.45 | 0.4101 | 1103.8 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.73 | 10.26 | 124.49 | 23.08 | 280.79 | 0.3943 | 1014.0 | 875.3 | |
| 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. | |