SDO HMI 2011-08-06 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.56 | 0.00 | 15.23 | 18.93 | 223.83 | -35.47 | 66.27 | 0.6012 | -323.6 | -246.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.81 | 0.00 | 1.05 | 18.11 | 229.46 | -29.84 | 64.97 | 0.5240 | -702.0 | -536.2 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 19.00 | 226.84 | -32.46 | 64.84 | 0.5628 | -765.0 | -588.9 | |
| 0.00 | 1.63 | 0.00 | 0.98 | 19.75 | 226.60 | -32.70 | 63.72 | 0.5693 | -747.0 | -515.5 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 19.20 | 226.34 | -32.96 | 64.77 | 0.5701 | -825.0 | -661.8 | |
| 0.00 | 2.44 | 0.00 | 1.49 | 20.44 | 225.50 | -33.80 | 63.15 | 0.5864 | -496.0 | -491.5 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 20.06 | 225.48 | -33.82 | 63.78 | 0.5850 | -682.0 | -536.8 | |
| 0.00 | 1.26 | 0.00 | 0.78 | 20.38 | 224.93 | -34.37 | 63.55 | 0.5933 | -515.0 | -449.0 | |
| 0.00 | 4.61 | 0.00 | 2.84 | 17.77 | 223.91 | -35.39 | 68.22 | 0.5961 | -869.0 | -656.9 | |
| 0.00 | 1.08 | 0.00 | 0.67 | 18.37 | 223.41 | -35.89 | 67.45 | 0.6046 | -766.0 | -686.8 | |
| 0.00 | 0.99 | 0.00 | 0.64 | 20.02 | 221.20 | -38.10 | 65.74 | 0.6382 | -631.0 | -518.3 | |
| 0.00 | 1.26 | 0.00 | 0.81 | 19.16 | 221.03 | -38.27 | 67.12 | 0.6373 | 757.0 | 650.2 | |
| 0.00 | 0.99 | 0.00 | 0.64 | 19.03 | 220.49 | -38.81 | 67.51 | 0.6436 | 529.0 | 477.1 | |
| 0.00 | 2.62 | 0.00 | 1.69 | 18.89 | 220.32 | -38.98 | 67.77 | 0.6452 | 712.0 | 549.3 | |
| 0.00 | 2.35 | 0.00 | 1.51 | 17.93 | 220.49 | -38.80 | 69.18 | 0.6401 | 470.0 | 370.3 | |
| 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. | |