SDO HMI 2014-10-05 18:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.26 | 27.13 | 4.88 | 15.90 | 14.28 | 90.48 | -31.58 | 73.70 | 0.5320 | 394.7 | 298.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.51 | 9.80 | 102.41 | -19.66 | 79.04 | 0.3392 | -734.0 | -611.1 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 9.22 | 97.79 | -24.28 | 81.94 | 0.4116 | -687.0 | -533.3 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 10.50 | 97.45 | -24.61 | 78.95 | 0.4190 | -770.0 | -565.3 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 10.28 | 96.70 | -25.37 | 79.67 | 0.4303 | -684.0 | -554.6 | |
| 0.00 | 1.58 | 0.00 | 0.91 | 17.41 | 92.44 | -29.62 | 66.66 | 0.5158 | 562.0 | 476.1 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 16.49 | 89.64 | -32.42 | 69.67 | 0.5504 | 636.0 | 451.6 | |
| 0.00 | 1.49 | 0.00 | 0.89 | 16.54 | 89.41 | -32.65 | 69.68 | 0.5537 | 691.0 | 614.5 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 18.90 | 88.85 | -33.22 | 65.85 | 0.5702 | 748.0 | 630.5 | |
| 3.34 | 13.70 | 1.97 | 8.10 | 13.33 | 89.25 | -32.81 | 75.47 | 0.5468 | 1123.9 | 669.2 | |
| 1.67 | -9.00 | 0.99 | -9.00 | 13.48 | 89.19 | -32.87 | 75.22 | 0.5480 | 799.2 | 999999 | |
| 3.25 | -9.00 | 1.92 | -9.00 | 13.18 | 89.20 | -32.86 | 75.76 | 0.5472 | 970.8 | 999999 | |
| 0.00 | 1.67 | 0.00 | 1.07 | 24.70 | 85.70 | -36.36 | 58.32 | 0.6353 | 478.0 | 354.2 | |
| 0.00 | 1.23 | 0.00 | 0.74 | 12.97 | 87.27 | -34.79 | 76.60 | 0.5738 | 521.0 | 434.6 | |
| 0.00 | 0.61 | 0.00 | 0.37 | 12.91 | 86.90 | -35.16 | 76.77 | 0.5788 | 638.0 | 439.6 | |
| 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. | |