SDO HMI 2011-06-02 02:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.47 | 170.10 | 17.84 | 102.65 | -20.53 | 19.37 | -29.45 | 126.64 | 0.5759 | 660.6 | 448.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.08 | 0.00 | 1.21 | -20.20 | 23.29 | -25.53 | 129.77 | 0.5284 | -826.0 | -649.0 | |
| 0.00 | 1.90 | 0.00 | 1.11 | -19.39 | 22.31 | -26.51 | 127.53 | 0.5329 | -910.0 | -744.5 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -19.07 | 22.26 | -26.56 | 126.97 | 0.5310 | -715.0 | -553.9 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -18.84 | 21.69 | -27.13 | 126.07 | 0.5361 | -877.0 | -650.4 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -18.24 | 21.47 | -27.35 | 124.89 | 0.5341 | -470.0 | -393.6 | |
| 23.86 | 151.30 | 14.42 | 91.29 | -20.48 | 19.43 | -29.39 | 126.60 | 0.5749 | 1140.0 | 506.0 | |
| 3.89 | -6.00 | 2.37 | -6.00 | -20.80 | 18.80 | -30.03 | 126.56 | 0.5845 | 741.1 | 999999 | |
| 1.72 | 2.53 | 1.05 | 1.55 | -21.35 | 18.56 | -30.26 | 127.17 | 0.5912 | 641.3 | 778.7 | |
| 0.00 | 2.71 | 0.00 | 1.66 | -21.06 | 18.32 | -30.50 | 126.55 | 0.5917 | 632.0 | 547.1 | |
| 0.00 | 1.36 | 0.00 | 0.83 | -20.31 | 18.45 | -30.37 | 125.55 | 0.5850 | 640.0 | 458.3 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -21.25 | 17.33 | -31.50 | 126.04 | 0.6044 | 637.0 | 553.8 | |
| 0.00 | 1.45 | 0.00 | 0.91 | -22.29 | 16.91 | -31.91 | 127.21 | 0.6163 | 803.0 | 565.2 | |
| 0.00 | 0.81 | 0.00 | 0.51 | -22.68 | 16.38 | -32.44 | 127.35 | 0.6248 | 683.0 | 543.6 | |
| 0.00 | 1.08 | 0.00 | 0.69 | -22.32 | 16.24 | -32.58 | 126.74 | 0.6238 | 588.0 | 519.8 | |
| 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. | |