SDO HMI 2011-10-05 19:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.90 | 127.29 | 62.74 | 215.18 | -14.25 | 116.81 | -70.03 | 107.23 | 0.9540 | 131.1 | -138.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.50 | 54.70 | 16.54 | 84.05 | -14.03 | 119.50 | -67.34 | 107.55 | 0.9405 | 523.5 | -449.4 | |
| 0.97 | 12.99 | 1.44 | 19.56 | -14.11 | 118.79 | -68.05 | 107.48 | 0.9445 | 197.7 | -79.6 | |
| 6.85 | -2.00 | 10.25 | -2.00 | -13.84 | 118.63 | -68.22 | 107.16 | 0.9451 | 481.5 | 999999 | |
| 0.00 | 5.44 | 0.00 | 8.16 | -13.32 | 118.53 | -68.32 | 106.60 | 0.9450 | 392.0 | 360.8 | |
| 0.00 | 0.88 | 0.00 | 1.37 | -14.12 | 117.75 | -69.09 | 107.27 | 0.9501 | -350.0 | -312.6 | |
| 2.37 | -1.00 | 3.85 | -1.00 | -14.75 | 117.23 | -69.61 | 107.80 | 0.9534 | -636.4 | 999999 | |
| 7.99 | 9.83 | 12.43 | 15.32 | -13.70 | 117.86 | -68.99 | 106.86 | 0.9491 | 279.1 | 136.3 | |
| 0.00 | 1.14 | 0.00 | 1.86 | -13.66 | 116.81 | -70.03 | 106.60 | 0.9543 | -48.0 | -92.2 | |
| 1.05 | 3.51 | 1.92 | 6.40 | -15.44 | 115.27 | -71.57 | 108.11 | 0.9633 | -132.4 | -17.4 | |
| 0.00 | 4.30 | 0.00 | 7.40 | -13.52 | 115.78 | -71.06 | 106.25 | 0.9592 | -396.0 | -339.1 | |
| 2.99 | 4.39 | 5.79 | 8.49 | -15.03 | 114.08 | -72.77 | 107.46 | 0.9681 | -236.1 | -301.1 | |
| 0.00 | 0.61 | 0.00 | 1.19 | -14.54 | 113.97 | -72.87 | 106.94 | 0.9681 | -505.0 | -452.3 | |
| 3.78 | 29.50 | 7.67 | 61.38 | -14.73 | 113.37 | -73.48 | 107.02 | 0.9707 | -336.8 | 184.6 | |
| 1.40 | -13.00 | 2.85 | -13.00 | -14.37 | 113.25 | -73.59 | 106.63 | 0.9709 | -317.9 | 999999 | |
| 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. | |