SDO HMI 2011-10-05 11:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.98 | 206.40 | 21.39 | 110.38 | -11.71 | 178.66 | -12.60 | 145.56 | 0.3782 | 479.5 | 282.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.81 | 173.80 | 1.50 | 92.59 | -11.93 | 179.48 | -11.77 | 147.55 | 0.3736 | 826.3 | 444.9 | |
| 31.98 | -1.00 | 17.04 | -1.00 | -11.50 | 179.25 | -12.00 | 146.39 | 0.3697 | 1211.3 | 999999 | |
| 0.62 | 4.48 | 0.33 | 2.40 | -12.05 | 178.47 | -12.78 | 145.56 | 0.3841 | 774.7 | 525.6 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -12.34 | 177.26 | -13.99 | 143.54 | 0.3992 | -672.0 | -448.2 | |
| 0.00 | 10.81 | 0.00 | 5.86 | -12.71 | 176.67 | -14.58 | 142.96 | 0.4094 | -1021.0 | -776.3 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -13.06 | 176.46 | -14.80 | 143.09 | 0.4160 | -728.0 | -515.3 | |
| 0.00 | 2.11 | 0.00 | 1.17 | -14.22 | 174.23 | -17.03 | 140.88 | 0.4517 | -818.0 | -596.7 | |
| 1.67 | 4.48 | 0.92 | 2.46 | -12.14 | 173.64 | -17.62 | 136.75 | 0.4336 | -980.1 | -830.8 | |
| 2.90 | 3.87 | 1.60 | 2.13 | -12.55 | 173.58 | -17.68 | 137.31 | 0.4389 | -920.3 | -693.4 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -13.13 | 173.34 | -17.91 | 137.83 | 0.4480 | -782.0 | -676.5 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -12.83 | 172.97 | -18.28 | 136.78 | 0.4484 | -702.0 | -501.9 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -11.88 | 172.27 | -18.99 | 134.17 | 0.4457 | -741.0 | -553.1 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -12.29 | 172.24 | -19.02 | 134.79 | 0.4505 | -499.0 | -403.9 | |
| 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. | |