SDO HMI 2010-08-11 16:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.17 | 81.81 | 26.79 | 47.48 | 14.25 | 301.51 | -30.90 | 73.09 | 0.5221 | -207.6 | 43.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.52 | 22.73 | 8.85 | 12.96 | 14.05 | 303.22 | -29.19 | 72.83 | 0.4971 | -848.9 | -181.7 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 14.38 | 302.56 | -29.85 | 72.45 | 0.5076 | 488.0 | 329.2 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 14.16 | 302.34 | -30.07 | 72.97 | 0.5101 | -837.0 | -621.4 | |
| 0.90 | 1.26 | 0.52 | 0.73 | 14.03 | 302.25 | -30.16 | 73.25 | 0.5110 | -782.6 | -726.2 | |
| 8.30 | 9.92 | 4.79 | 5.73 | 14.23 | 302.00 | -30.41 | 72.96 | 0.5151 | -850.9 | -655.1 | |
| 0.00 | 1.44 | 0.00 | 0.83 | 13.95 | 302.04 | -30.36 | 73.47 | 0.5138 | -176.0 | -292.2 | |
| 3.61 | 12.99 | 2.10 | 7.56 | 14.41 | 301.42 | -30.98 | 72.82 | 0.5239 | -816.0 | -536.4 | |
| 1.80 | -7.00 | 1.05 | -7.00 | 14.48 | 301.01 | -31.40 | 72.85 | 0.5299 | -520.8 | 999999 | |
| 1.62 | 13.62 | 0.95 | 7.96 | 13.64 | 300.77 | -31.63 | 74.50 | 0.5310 | 873.4 | 555.6 | |
| 1.35 | -9.00 | 0.79 | -9.00 | 13.84 | 300.59 | -31.81 | 74.17 | 0.5341 | 808.5 | 999999 | |
| 1.17 | 2.17 | 0.69 | 1.27 | 14.74 | 300.19 | -32.22 | 72.66 | 0.5422 | 674.4 | 731.0 | |
| 0.00 | 1.35 | 0.00 | 0.80 | 14.70 | 299.97 | -32.43 | 72.81 | 0.5451 | 743.0 | 600.8 | |
| 9.83 | 11.46 | 5.82 | 6.79 | 15.05 | 299.69 | -32.72 | 72.27 | 0.5501 | 828.8 | 548.9 | |
| 2.07 | 2.89 | 1.23 | 1.71 | 13.86 | 299.40 | -33.00 | 74.50 | 0.5509 | 723.5 | 600.6 | |
| 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. | |