SDO HMI 2014-10-09 16:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.94 | 0.00 | 9.14 | 13.19 | 61.31 | -9.09 | 47.39 | 0.2054 | -278.6 | -214.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.93 | 0.00 | 0.97 | 14.22 | 67.18 | -3.22 | 21.40 | 0.1498 | -989.0 | -830.3 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 14.22 | 66.87 | -3.53 | 23.24 | 0.1518 | -910.0 | -786.3 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 7.97 | 65.96 | -4.43 | 68.42 | 0.0826 | 833.0 | 518.7 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 12.94 | 65.16 | -5.23 | 37.24 | 0.1476 | -845.0 | -670.6 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 12.37 | 65.11 | -5.28 | 40.04 | 0.1405 | -978.0 | -794.1 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 12.16 | 64.99 | -5.40 | 41.68 | 0.1391 | -839.0 | -714.7 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 15.89 | 63.40 | -6.99 | 34.83 | 0.2058 | -812.0 | -625.8 | |
| 0.00 | 1.66 | 0.00 | 0.84 | 14.82 | 63.16 | -7.24 | 39.09 | 0.1940 | -953.0 | -835.6 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 13.71 | 63.19 | -7.20 | 43.00 | 0.1794 | -883.0 | -705.3 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 13.97 | 62.28 | -8.11 | 45.34 | 0.1934 | -914.0 | -714.4 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 13.77 | 58.22 | -12.18 | 56.94 | 0.2455 | 907.0 | 655.8 | |
| 0.00 | 1.84 | 0.00 | 0.96 | 12.36 | 53.51 | -16.89 | 68.64 | 0.3060 | 954.0 | 723.7 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 12.11 | 52.40 | -17.99 | 70.44 | 0.3220 | 866.0 | 682.2 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 14.37 | 48.74 | -21.65 | 67.41 | 0.3888 | 662.0 | 584.3 | |
| 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. | |