SDO HMI 2011-10-08 14:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.38 | 0.00 | 10.27 | -14.17 | 146.24 | -3.78 | 169.60 | 0.3591 | 122.4 | 141.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.74 | -14.66 | 148.74 | -1.28 | 176.54 | 0.3604 | 817.0 | 648.2 | |
| 0.00 | 2.28 | 0.00 | 1.22 | -15.63 | 148.39 | -1.63 | 175.80 | 0.3764 | 691.0 | 564.7 | |
| 0.00 | 1.49 | 0.00 | 0.79 | -14.70 | 148.33 | -1.69 | 175.46 | 0.3614 | 799.0 | 625.5 | |
| 0.00 | 2.37 | 0.00 | 1.26 | -14.99 | 148.11 | -1.91 | 174.95 | 0.3664 | 890.0 | 668.9 | |
| 0.00 | 1.58 | 0.00 | 0.83 | -13.67 | 147.94 | -2.08 | 174.11 | 0.3452 | 919.0 | 676.9 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -14.57 | 147.44 | -2.58 | 173.02 | 0.3608 | 782.0 | 580.5 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -12.10 | 145.50 | -4.52 | 166.29 | 0.3265 | -907.0 | -687.2 | |
| 0.00 | 1.58 | 0.00 | 0.83 | -12.45 | 145.34 | -4.68 | 166.08 | 0.3327 | -762.0 | -685.8 | |
| 0.00 | 0.44 | 0.00 | 0.23 | -15.37 | 144.28 | -5.74 | 165.36 | 0.3832 | 829.0 | 697.8 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -15.41 | 144.03 | -5.99 | 164.78 | 0.3847 | 729.0 | 572.3 | |
| 0.00 | 0.70 | 0.00 | 0.37 | -13.52 | 143.43 | -6.59 | 161.78 | 0.3582 | -662.0 | -515.4 | |
| 0.00 | 1.75 | 0.00 | 0.93 | -13.53 | 143.09 | -6.93 | 160.90 | 0.3601 | -823.0 | -626.9 | |
| 0.00 | 0.61 | 0.00 | 0.33 | -13.28 | 142.85 | -7.17 | 160.05 | 0.3575 | -765.0 | -602.3 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -13.76 | 142.53 | -7.50 | 159.70 | 0.3667 | -823.0 | -709.9 | |
| 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. | |