SDO HMI 2011-06-07 08:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.75 | 156.72 | 17.97 | 79.01 | 9.74 | 336.16 | -3.20 | 8.81 | 0.1802 | -792.1 | -358.5 | |
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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 | 0.72 | 6.27 | 342.38 | 3.02 | 334.20 | 0.1207 | -965.0 | -623.0 | |
| 0.00 | 1.99 | 0.00 | 1.00 | 7.80 | 339.38 | 0.02 | 359.89 | 0.1353 | -976.0 | -841.1 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 8.57 | 337.16 | -2.20 | 14.39 | 0.1535 | -1045.0 | -812.8 | |
| 33.04 | 126.46 | 16.61 | 63.58 | 9.46 | 336.94 | -2.42 | 14.31 | 0.1694 | -1357.7 | -396.3 | |
| 0.36 | 3.35 | 0.18 | 1.68 | 7.96 | 336.37 | -3.00 | 20.65 | 0.1475 | -1213.0 | -947.6 | |
| 2.35 | 2.53 | 1.18 | 1.27 | 8.69 | 336.21 | -3.16 | 19.93 | 0.1604 | -987.8 | -870.3 | |
| 0.00 | 2.72 | 0.00 | 1.36 | 8.20 | 335.41 | -3.95 | 25.72 | 0.1579 | -944.0 | -794.3 | |
| 0.00 | 2.72 | 0.00 | 1.37 | 10.64 | 335.23 | -4.14 | 21.11 | 0.1976 | -650.0 | -604.1 | |
| 0.00 | 2.35 | 0.00 | 1.19 | 9.25 | 333.70 | -5.66 | 31.39 | 0.1879 | -936.0 | -685.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 15.92 | 330.29 | -9.07 | 29.01 | 0.3139 | 889.0 | 624.7 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 14.57 | 329.62 | -9.74 | 33.18 | 0.3006 | 815.0 | 653.2 | |
| 0.00 | 3.71 | 0.00 | 1.92 | 13.78 | 329.49 | -9.87 | 35.06 | 0.2910 | 719.0 | 545.7 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 15.54 | 327.90 | -11.46 | 35.64 | 0.3299 | 769.0 | 532.8 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 17.64 | 326.30 | -13.06 | 35.49 | 0.3725 | 924.0 | 762.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 11.44 | 325.17 | -14.19 | 50.60 | 0.3123 | -814.0 | -702.4 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 14.72 | 324.10 | -15.26 | 45.17 | 0.3606 | 863.0 | 690.8 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 12.66 | 320.88 | -18.48 | 54.81 | 0.3801 | 382.0 | 399.0 | |
| 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. | |