SDO HMI 2011-08-24 17:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.94 | 0.00 | 11.66 | 18.76 | 357.63 | -24.84 | 61.34 | 0.4527 | -446.8 | -334.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.49 | 20.68 | 1.97 | -20.50 | 53.36 | 0.4100 | -805.0 | -598.3 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 17.29 | 1.87 | -20.61 | 61.04 | 0.3857 | -797.0 | -597.4 | |
| 0.00 | 1.26 | 0.00 | 0.69 | 20.49 | 1.10 | -21.37 | 54.78 | 0.4196 | -861.0 | -661.3 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 19.62 | 0.43 | -22.04 | 57.33 | 0.4218 | -967.0 | -797.4 | |
| 0.00 | 2.06 | 0.00 | 1.11 | 16.71 | 0.61 | -21.87 | 63.61 | 0.3999 | -927.0 | -750.4 | |
| 0.00 | 3.68 | 0.00 | 2.01 | 18.57 | 359.89 | -22.59 | 60.11 | 0.4217 | -670.0 | -586.2 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 18.44 | 359.73 | -22.74 | 60.54 | 0.4230 | -765.0 | -667.3 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 18.40 | 359.60 | -22.88 | 60.74 | 0.4246 | -515.0 | -430.9 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 16.45 | 359.55 | -22.93 | 65.11 | 0.4136 | -775.0 | -679.6 | |
| 0.00 | 1.62 | 0.00 | 0.89 | 19.30 | 358.38 | -24.09 | 59.93 | 0.4470 | -698.0 | -447.9 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 15.68 | 358.27 | -24.21 | 67.79 | 0.4282 | -570.0 | -475.0 | |
| 0.00 | 2.24 | 0.00 | 1.28 | 17.91 | 354.19 | -28.29 | 65.77 | 0.4965 | 849.0 | 670.2 | |
| 0.00 | 1.08 | 0.00 | 0.67 | 22.11 | 347.59 | -34.89 | 62.08 | 0.6019 | 720.0 | 625.3 | |
| 0.00 | 1.26 | 0.00 | 0.81 | 22.14 | 344.48 | -38.00 | 63.44 | 0.6398 | 526.0 | 404.1 | |
| 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. | |