SDO HMI 2014-10-12 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.78 | 0.00 | 12.29 | 13.35 | 56.93 | 27.77 | 287.32 | 0.4755 | 101.6 | 282.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.82 | 12.16 | 66.43 | 37.27 | 282.15 | 0.6078 | -662.0 | -561.5 | |
| 0.00 | 0.70 | 0.00 | 0.44 | 13.08 | 66.24 | 37.08 | 283.70 | 0.6067 | -666.0 | -601.1 | |
| 0.00 | 1.31 | 0.00 | 0.79 | 10.28 | 63.74 | 34.58 | 279.35 | 0.5681 | -655.0 | -520.7 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 16.35 | 59.08 | 29.92 | 291.89 | 0.5178 | -757.0 | -600.0 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 16.23 | 59.02 | 29.86 | 291.70 | 0.5166 | -792.0 | -733.6 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 16.51 | 59.03 | 29.87 | 292.20 | 0.5178 | -696.0 | -504.0 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 13.20 | 58.35 | 29.19 | 286.15 | 0.4963 | 678.0 | 504.4 | |
| 0.00 | 0.79 | 0.00 | 0.44 | 13.18 | 55.70 | 26.54 | 287.23 | 0.4574 | 647.0 | 523.1 | |
| 0.00 | 0.79 | 0.00 | 0.44 | 13.59 | 55.37 | 26.21 | 288.26 | 0.4540 | 571.0 | 472.3 | |
| 0.00 | 4.11 | 0.00 | 2.28 | 13.29 | 55.30 | 26.14 | 287.65 | 0.4519 | 784.0 | 620.0 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 13.79 | 54.99 | 25.83 | 288.90 | 0.4491 | 572.0 | 486.4 | |
| 0.00 | 5.86 | 0.00 | 3.24 | 13.65 | 54.80 | 25.64 | 288.69 | 0.4457 | 712.0 | 607.7 | |
| 0.00 | 1.92 | 0.00 | 1.05 | 13.45 | 53.82 | 24.66 | 288.79 | 0.4305 | 858.0 | 568.9 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 11.24 | 49.67 | 20.51 | 285.74 | 0.3586 | 828.0 | 697.3 | |
| 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. | |