SDO HMI 2011-10-13 05:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.88 | 33.18 | 4.26 | 18.14 | 20.39 | 109.85 | 20.86 | 307.30 | 0.4213 | 418.0 | 322.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.53 | 0.00 | 0.30 | 25.21 | 114.26 | 25.27 | 311.16 | 0.5151 | 618.0 | 533.3 | |
| 0.00 | 2.54 | 0.00 | 1.46 | 25.38 | 114.08 | 25.09 | 311.61 | 0.5144 | 598.0 | 554.2 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 19.95 | 112.62 | 23.63 | 303.44 | 0.4534 | -692.0 | -556.8 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 20.84 | 112.70 | 23.71 | 305.09 | 0.4611 | -799.0 | -677.5 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 24.18 | 112.96 | 23.97 | 310.80 | 0.4915 | 593.0 | 587.2 | |
| 0.00 | 2.01 | 0.00 | 1.11 | 20.61 | 110.79 | 21.80 | 306.67 | 0.4351 | -997.0 | -819.0 | |
| 0.00 | 2.54 | 0.00 | 1.39 | 19.94 | 110.45 | 21.46 | 305.71 | 0.4253 | -833.0 | -632.7 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 19.41 | 109.83 | 20.84 | 305.33 | 0.4130 | 678.0 | 516.0 | |
| 2.80 | 5.25 | 1.52 | 2.85 | 19.39 | 109.35 | 20.36 | 305.87 | 0.4067 | 863.3 | 720.3 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 20.53 | 109.47 | 20.48 | 308.07 | 0.4180 | 655.0 | 537.8 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 18.44 | 109.16 | 20.17 | 304.05 | 0.3966 | 820.0 | 661.9 | |
| 0.00 | 1.93 | 0.00 | 1.04 | 19.59 | 108.97 | 19.98 | 306.75 | 0.4035 | 929.0 | 682.4 | |
| 0.00 | 3.06 | 0.00 | 1.66 | 20.24 | 108.92 | 19.93 | 308.17 | 0.4086 | 742.0 | 742.6 | |
| 5.08 | 8.84 | 2.74 | 4.77 | 19.54 | 108.49 | 19.50 | 307.27 | 0.3970 | 1063.5 | 859.6 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 21.62 | 105.45 | 16.46 | 316.00 | 0.3809 | 677.0 | 514.7 | |
| 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. | |