SDO HMI 2011-06-13 03:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.81 | 22.66 | 0.99 | 12.24 | -15.73 | 245.99 | -16.70 | 136.18 | 0.3983 | 282.0 | 300.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.76 | -15.11 | 250.69 | -11.99 | 143.71 | 0.3403 | 923.0 | 652.6 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -15.27 | 250.49 | -12.19 | 143.54 | 0.3444 | 884.0 | 711.2 | |
| 0.00 | 2.27 | 0.00 | 1.19 | -15.02 | 250.35 | -12.34 | 142.76 | 0.3426 | 1105.0 | 730.4 | |
| 0.00 | 2.08 | 0.00 | 1.11 | -14.74 | 247.61 | -15.08 | 136.68 | 0.3683 | 1008.0 | 766.5 | |
| 0.00 | 1.81 | 0.00 | 0.97 | -15.60 | 247.25 | -15.44 | 137.64 | 0.3821 | 865.0 | 744.2 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -15.32 | 247.27 | -15.42 | 137.15 | 0.3786 | 859.0 | 622.8 | |
| 0.00 | 0.91 | 0.00 | 0.49 | -15.51 | 246.99 | -15.69 | 137.00 | 0.3838 | 722.0 | 623.6 | |
| 0.00 | 1.63 | 0.00 | 0.88 | -14.82 | 245.60 | -17.08 | 133.32 | 0.3920 | 734.0 | 709.3 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -18.98 | 243.51 | -19.18 | 137.33 | 0.4602 | 605.0 | 449.9 | |
| 1.81 | 2.18 | 0.99 | 1.19 | -15.11 | 243.65 | -19.03 | 130.89 | 0.4182 | -879.5 | -753.0 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -16.16 | 242.40 | -20.28 | 131.08 | 0.4435 | -730.0 | -559.2 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -16.90 | 242.29 | -20.40 | 132.20 | 0.4520 | -831.0 | -596.6 | |
| 0.00 | 1.99 | 0.00 | 1.11 | -16.80 | 241.58 | -21.10 | 131.12 | 0.4593 | -743.0 | -640.5 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -16.20 | 241.65 | -21.03 | 130.15 | 0.4527 | -585.0 | -483.6 | |
| 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. | |