SDO HMI 2014-10-04 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.16 | 30.82 | 7.87 | 21.24 | 13.55 | 90.69 | -44.02 | 77.34 | 0.6931 | 307.4 | 119.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.45 | 11.94 | 105.86 | -28.84 | 77.12 | 0.4861 | 760.0 | 626.2 | |
| 0.00 | 0.26 | 0.00 | 0.15 | 10.84 | 102.94 | -31.77 | 79.94 | 0.5272 | -555.0 | -575.3 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 14.42 | 97.18 | -37.52 | 74.83 | 0.6134 | -740.0 | -598.7 | |
| 0.00 | 1.41 | 0.00 | 0.88 | 14.50 | 96.97 | -37.73 | 74.75 | 0.6164 | -590.0 | -492.7 | |
| 0.00 | 2.64 | 0.00 | 1.64 | 10.76 | 97.19 | -37.52 | 80.83 | 0.6083 | -717.0 | -483.4 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 7.98 | 97.11 | -37.59 | 85.42 | 0.6083 | -815.0 | -658.8 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 7.86 | 97.09 | -37.62 | 85.62 | 0.6087 | -746.0 | -489.6 | |
| 0.00 | 1.14 | 0.00 | 0.81 | 16.58 | 88.92 | -45.79 | 73.21 | 0.7199 | 438.0 | 420.8 | |
| 11.16 | 15.99 | 7.87 | 11.28 | 13.28 | 89.06 | -45.65 | 77.78 | 0.7144 | 852.3 | 491.7 | |
| 0.00 | 1.58 | 0.00 | 1.12 | 13.52 | 88.60 | -46.10 | 77.49 | 0.7200 | 446.0 | 349.1 | |
| 0.00 | 0.53 | 0.00 | 0.38 | 14.97 | 87.26 | -47.45 | 75.64 | 0.7369 | 630.0 | 547.2 | |
| 0.00 | 0.79 | 0.00 | 0.58 | 14.92 | 87.09 | -47.62 | 75.72 | 0.7388 | 512.0 | 501.7 | |
| 0.00 | 1.05 | 0.00 | 0.77 | 14.54 | 86.92 | -47.79 | 76.26 | 0.7404 | 507.0 | 454.3 | |
| 0.00 | 1.49 | 0.00 | 1.20 | 22.05 | 83.05 | -51.65 | 67.08 | 0.7915 | 579.0 | 436.2 | |
| 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. | |