SDO HMI 2014-10-08 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.13 | 0.00 | 13.40 | 10.75 | 97.31 | 12.07 | 232.80 | 0.2514 | -407.8 | -417.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.73 | 9.49 | 103.92 | 18.68 | 280.97 | 0.3232 | -884.0 | -869.7 | |
| 0.00 | 2.28 | 0.00 | 1.19 | 8.93 | 103.76 | 18.52 | 279.28 | 0.3194 | -975.0 | -707.9 | |
| 0.00 | 3.25 | 0.00 | 1.69 | 8.67 | 103.52 | 18.28 | 278.54 | 0.3150 | -878.0 | -693.5 | |
| 0.00 | 1.84 | 0.00 | 0.96 | 9.45 | 102.51 | 17.27 | 281.51 | 0.3002 | 1013.0 | 762.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 10.44 | 100.60 | 15.36 | 286.25 | 0.2726 | -735.0 | -602.5 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 10.12 | 100.23 | 15.00 | 285.40 | 0.2654 | -855.0 | -640.2 | |
| 0.00 | 5.35 | 0.00 | 2.73 | 10.31 | 98.92 | 13.69 | 287.37 | 0.2450 | -636.0 | -839.1 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 10.05 | 98.69 | 13.46 | 286.55 | 0.2401 | -702.0 | -636.5 | |
| 0.00 | 1.93 | 0.00 | 0.98 | 11.19 | 97.59 | 12.35 | 292.63 | 0.2284 | -756.0 | -621.2 | |
| 0.00 | 2.19 | 0.00 | 1.11 | 8.40 | 97.32 | 12.09 | 280.63 | 0.2117 | -780.0 | -569.1 | |
| 0.00 | 2.63 | 0.00 | 1.32 | 14.99 | 84.17 | -1.06 | 6.78 | 0.1527 | 878.0 | 680.0 | |
| 0.00 | 1.32 | 0.00 | 0.65 | 10.68 | 83.79 | -1.45 | 18.03 | 0.0806 | -785.0 | -649.3 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 22.54 | 78.67 | -6.56 | 20.65 | 0.3007 | 794.0 | 600.8 | |
| 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. | |