SDO HMI 2011-10-24 01:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.79 | 0.00 | 13.14 | 23.96 | 331.12 | 25.03 | 310.65 | 0.5123 | -521.2 | -456.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.69 | 21.37 | 338.66 | 32.57 | 300.22 | 0.5824 | -706.0 | -595.6 | |
| 0.00 | 1.13 | 0.00 | 0.67 | 22.33 | 336.15 | 30.06 | 303.45 | 0.5574 | -689.0 | -571.0 | |
| 0.00 | 2.17 | 0.00 | 1.29 | 21.84 | 335.92 | 29.83 | 302.82 | 0.5516 | -342.0 | -274.6 | |
| 0.00 | 0.61 | 0.00 | 0.35 | 21.33 | 332.21 | 26.12 | 304.96 | 0.5025 | -712.0 | -594.1 | |
| 0.00 | 1.22 | 0.00 | 0.70 | 22.56 | 331.20 | 25.11 | 308.03 | 0.4996 | -870.0 | -737.8 | |
| 0.00 | 1.13 | 0.00 | 0.65 | 24.36 | 330.24 | 24.15 | 312.01 | 0.5036 | -657.0 | -523.1 | |
| 0.00 | 1.83 | 0.00 | 1.04 | 24.14 | 330.16 | 24.07 | 311.74 | 0.5008 | -780.0 | -630.6 | |
| 0.00 | 2.17 | 0.00 | 1.24 | 23.49 | 329.92 | 23.83 | 310.91 | 0.4923 | -785.0 | -582.7 | |
| 0.00 | 1.39 | 0.00 | 0.79 | 23.93 | 329.76 | 23.67 | 311.83 | 0.4944 | -873.0 | -751.7 | |
| 0.00 | 2.96 | 0.00 | 1.68 | 23.71 | 329.72 | 23.63 | 311.51 | 0.4920 | -782.0 | -614.2 | |
| 0.00 | 1.57 | 0.00 | 0.90 | 24.91 | 329.88 | 23.79 | 313.28 | 0.5046 | -640.0 | -548.1 | |
| 0.00 | 2.96 | 0.00 | 1.69 | 24.66 | 329.80 | 23.71 | 312.97 | 0.5014 | -769.0 | -651.9 | |
| 0.00 | 1.48 | 0.00 | 0.86 | 27.67 | 329.13 | 23.04 | 318.28 | 0.5230 | 674.0 | 529.4 | |
| 0.00 | 1.04 | 0.00 | 0.59 | 28.71 | 324.92 | 18.83 | 324.94 | 0.4948 | 634.0 | 591.7 | |
| 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. | |