SDO HMI 2011-08-09 11:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.26 | 29.61 | 0.64 | 15.06 | 19.16 | 224.76 | 0.70 | 357.26 | 0.2261 | -600.0 | -571.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.50 | 17.45 | 229.83 | 5.77 | 333.67 | 0.2171 | -791.0 | -629.5 | |
| 0.00 | 4.25 | 0.00 | 2.17 | 20.56 | 226.39 | 2.33 | 351.22 | 0.2502 | -782.0 | -647.1 | |
| 1.26 | 6.05 | 0.64 | 3.08 | 19.62 | 225.89 | 1.83 | 352.56 | 0.2333 | -1034.1 | -870.7 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 20.72 | 225.90 | 1.84 | 353.11 | 0.2518 | -856.0 | -716.2 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 19.84 | 225.63 | 1.57 | 353.70 | 0.2365 | -802.0 | -727.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 20.00 | 225.51 | 1.45 | 354.28 | 0.2389 | -896.0 | -680.8 | |
| 0.00 | 2.98 | 0.00 | 1.51 | 17.88 | 224.27 | 0.21 | 358.98 | 0.2015 | -825.0 | -679.0 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 18.13 | 224.27 | 0.21 | 359.00 | 0.2058 | -1010.0 | -818.3 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.50 | 224.27 | 0.22 | 359.03 | 0.2122 | -886.0 | -731.6 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 18.35 | 223.73 | -0.33 | 1.50 | 0.2095 | -865.0 | -696.6 | |
| 0.00 | 3.88 | 0.00 | 1.97 | 18.38 | 223.38 | -0.68 | 3.09 | 0.2103 | -1018.0 | -761.2 | |
| 0.00 | 2.08 | 0.00 | 1.06 | 18.93 | 221.77 | -2.29 | 9.81 | 0.2228 | 937.0 | 790.9 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 18.69 | 218.36 | -5.70 | 23.63 | 0.2356 | 872.0 | 697.1 | |
| 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. | |