SDO HMI 2011-10-10 22:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.40 | 166.36 | 17.20 | 103.84 | 23.40 | 153.80 | 34.58 | 301.12 | 0.6106 | -420.8 | -326.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.04 | 152.54 | 3.80 | 95.68 | 23.00 | 154.71 | 35.49 | 299.92 | 0.6189 | -816.3 | -418.6 | |
| 0.26 | -1.00 | 0.16 | -1.00 | 22.67 | 154.57 | 35.35 | 299.48 | 0.6155 | -820.7 | 999999 | |
| 21.10 | -1.00 | 13.24 | -1.00 | 23.28 | 154.31 | 35.09 | 300.55 | 0.6155 | -1102.9 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.37 | 25.26 | 150.07 | 30.85 | 306.28 | 0.5775 | 663.0 | 556.0 | |
| 0.00 | 1.75 | 0.00 | 1.05 | 25.70 | 148.35 | 29.13 | 308.28 | 0.5610 | 614.0 | 523.8 | |
| 0.00 | 1.75 | 0.00 | 1.03 | 23.48 | 147.75 | 28.53 | 305.20 | 0.5383 | 708.0 | 539.4 | |
| 0.00 | 0.96 | 0.00 | 0.57 | 25.83 | 147.70 | 28.48 | 309.01 | 0.5546 | 779.0 | 629.8 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 26.78 | 147.88 | 28.67 | 310.32 | 0.5638 | 548.0 | 459.1 | |
| 0.00 | 0.96 | 0.00 | 0.57 | 26.44 | 147.75 | 28.53 | 309.91 | 0.5597 | 647.0 | 475.5 | |
| 0.00 | 0.70 | 0.00 | 0.42 | 27.30 | 147.95 | 28.73 | 311.03 | 0.5685 | 587.0 | 384.0 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 26.74 | 145.34 | 26.12 | 312.54 | 0.5357 | 667.0 | 446.6 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 25.77 | 144.85 | 25.63 | 311.50 | 0.5221 | 830.0 | 679.7 | |
| 0.00 | 3.50 | 0.00 | 2.04 | 26.39 | 144.66 | 25.44 | 312.65 | 0.5253 | 747.0 | 652.3 | |
| 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. | |