SDO HMI 2011-09-06 18:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.98 | 25.94 | 5.17 | 21.87 | -19.21 | 258.02 | 47.83 | 239.85 | 0.8113 | 41.8 | 104.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.82 | 11.86 | 4.17 | 10.24 | -19.39 | 259.19 | 48.99 | 240.22 | 0.8223 | 540.6 | 619.2 | |
| 1.16 | -1.00 | 1.00 | -1.00 | -19.53 | 258.95 | 48.76 | 239.95 | 0.8209 | 636.8 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.00 | -20.09 | 258.84 | 48.65 | 239.27 | 0.8222 | 365.0 | 308.5 | |
| 0.00 | 1.52 | 0.00 | 1.30 | -19.60 | 258.59 | 48.39 | 239.70 | 0.8180 | 595.0 | 495.2 | |
| 0.00 | 1.07 | 0.00 | 0.91 | -19.11 | 258.39 | 48.20 | 240.15 | 0.8143 | 674.0 | 624.7 | |
| 0.00 | 0.89 | 0.00 | 0.74 | -18.59 | 257.81 | 47.62 | 240.46 | 0.8070 | -340.0 | -259.5 | |
| 0.00 | 0.98 | 0.00 | 0.77 | -15.50 | 256.42 | 46.23 | 243.35 | 0.7808 | -527.0 | -436.4 | |
| 0.00 | 1.69 | 0.00 | 1.41 | -18.99 | 257.44 | 47.24 | 239.83 | 0.8053 | -186.0 | -160.5 | |
| 0.00 | 0.89 | 0.00 | 0.73 | -18.41 | 256.99 | 46.80 | 240.26 | 0.7988 | -519.0 | -414.8 | |
| 0.00 | 1.87 | 0.00 | 1.52 | -19.18 | 255.97 | 45.78 | 238.86 | 0.7930 | -396.0 | -338.3 | |
| 0.00 | 0.62 | 0.00 | 0.52 | -20.32 | 256.40 | 46.20 | 237.79 | 0.8022 | -305.0 | -237.0 | |
| 0.00 | 0.80 | 0.00 | 0.65 | -19.60 | 255.89 | 45.70 | 238.34 | 0.7943 | -419.0 | -344.3 | |
| 0.00 | 0.98 | 0.00 | 0.79 | -19.14 | 255.64 | 45.44 | 238.72 | 0.7898 | -633.0 | -522.3 | |
| 0.00 | 1.61 | 0.00 | 1.29 | -19.31 | 255.60 | 45.41 | 238.52 | 0.7903 | -483.0 | -447.2 | |
| 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. | |