SDO HMI 2014-10-12 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 | 18.72 | 0.00 | 10.52 | 13.61 | 57.79 | 26.97 | 288.62 | 0.4651 | 246.1 | 159.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.19 | 0.00 | 1.34 | 12.13 | 66.74 | 35.93 | 282.33 | 0.5894 | -390.0 | -323.4 | |
| 0.00 | 1.57 | 0.00 | 0.96 | 11.54 | 66.50 | 35.69 | 281.37 | 0.5852 | -693.0 | -542.8 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 11.68 | 60.80 | 29.99 | 282.88 | 0.5041 | 708.0 | 534.3 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 13.33 | 59.29 | 28.47 | 286.69 | 0.4863 | 630.0 | 538.8 | |
| 0.00 | 0.44 | 0.00 | 0.25 | 16.53 | 59.69 | 28.87 | 292.78 | 0.5041 | -605.0 | -551.8 | |
| 0.00 | 1.49 | 0.00 | 0.85 | 15.70 | 59.17 | 28.35 | 291.47 | 0.4932 | -604.0 | -465.8 | |
| 0.00 | 1.66 | 0.00 | 0.93 | 17.16 | 56.86 | 26.05 | 295.80 | 0.4679 | -733.0 | -608.1 | |
| 0.00 | 2.54 | 0.00 | 1.39 | 13.24 | 55.42 | 24.61 | 288.35 | 0.4289 | 817.0 | 652.2 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 12.85 | 55.35 | 24.53 | 287.50 | 0.4263 | 643.0 | 499.4 | |
| 0.00 | 2.54 | 0.00 | 1.39 | 13.66 | 54.89 | 24.08 | 289.61 | 0.4227 | 633.0 | 608.9 | |
| 0.00 | 0.87 | 0.00 | 0.47 | 13.49 | 53.77 | 22.95 | 289.94 | 0.4051 | 757.0 | 627.9 | |
| 0.00 | 1.22 | 0.00 | 0.66 | 11.76 | 53.37 | 22.56 | 285.95 | 0.3922 | 704.0 | 572.8 | |
| 0.00 | 1.22 | 0.00 | 0.65 | 15.00 | 49.95 | 19.13 | 296.98 | 0.3568 | 826.0 | 662.1 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 13.98 | 49.50 | 18.68 | 294.77 | 0.3438 | 753.0 | 567.2 | |
| 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. | |