SDO HMI 2014-10-04 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.84 | 29.18 | 6.82 | 19.60 | 13.53 | 91.30 | -42.30 | 77.21 | 0.6710 | 240.8 | 128.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.74 | 12.09 | 105.86 | -27.74 | 76.47 | 0.4701 | 542.0 | 576.9 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 10.29 | 102.65 | -30.95 | 80.87 | 0.5145 | -661.0 | -546.8 | |
| 0.00 | 1.76 | 0.00 | 1.02 | 9.37 | 102.36 | -31.25 | 82.69 | 0.5180 | -584.0 | -351.3 | |
| 0.00 | 1.41 | 0.00 | 0.84 | 12.42 | 99.29 | -34.31 | 77.53 | 0.5660 | -741.0 | -579.2 | |
| 0.00 | 1.23 | 0.00 | 0.76 | 14.43 | 96.98 | -36.62 | 74.62 | 0.6014 | -618.0 | -519.3 | |
| 0.00 | 1.23 | 0.00 | 0.75 | 7.91 | 97.16 | -36.44 | 85.54 | 0.5923 | -783.0 | -541.6 | |
| 0.00 | 1.23 | 0.00 | 0.76 | 8.03 | 96.73 | -36.87 | 85.33 | 0.5983 | -533.0 | -490.4 | |
| 0.00 | 1.05 | 0.00 | 0.72 | 14.32 | 90.23 | -43.37 | 76.04 | 0.6879 | -578.0 | -484.3 | |
| 0.00 | 1.23 | 0.00 | 0.86 | 16.66 | 88.91 | -44.69 | 72.90 | 0.7073 | 514.0 | 443.8 | |
| 9.84 | 13.71 | 6.82 | 9.50 | 13.28 | 89.01 | -44.59 | 77.69 | 0.7017 | 865.0 | 581.8 | |
| 0.00 | 0.79 | 0.00 | 0.55 | 13.43 | 88.63 | -44.97 | 77.51 | 0.7064 | 470.0 | 380.9 | |
| 0.00 | 1.41 | 0.00 | 1.01 | 14.86 | 87.06 | -46.54 | 75.68 | 0.7264 | 687.0 | 634.5 | |
| 0.00 | 0.70 | 0.00 | 0.50 | 14.65 | 87.07 | -46.53 | 75.98 | 0.7260 | 590.0 | 509.6 | |
| 0.00 | 1.76 | 0.00 | 1.39 | 22.08 | 83.02 | -50.58 | 66.83 | 0.7809 | 568.0 | 468.4 | |
| 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. | |