SDO HMI 2011-10-09 14:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.29 | 219.50 | 18.10 | 119.23 | 23.42 | 154.56 | 17.73 | 317.09 | 0.4123 | -696.2 | -375.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.75 | 0.00 | 0.99 | 27.35 | 156.73 | 19.90 | 320.41 | 0.4763 | -637.0 | -535.5 | |
| 8.15 | 203.37 | 4.43 | 110.54 | 23.08 | 155.19 | 18.36 | 315.46 | 0.4149 | -1149.7 | -436.7 | |
| 23.74 | -2.00 | 12.91 | -2.00 | 23.34 | 154.85 | 18.02 | 316.44 | 0.4139 | -1385.3 | 999999 | |
| 1.40 | -2.00 | 0.76 | -2.00 | 22.95 | 154.55 | 17.72 | 316.15 | 0.4064 | -1342.9 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 22.69 | 152.75 | 15.93 | 318.54 | 0.3841 | 572.0 | 392.9 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 24.83 | 152.62 | 15.79 | 322.53 | 0.4076 | -833.0 | -673.2 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 24.89 | 151.60 | 14.77 | 324.37 | 0.3987 | -782.0 | -568.2 | |
| 0.00 | 2.28 | 0.00 | 1.23 | 25.43 | 150.09 | 13.26 | 327.95 | 0.3922 | 650.0 | 566.3 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 26.78 | 149.90 | 13.08 | 330.22 | 0.4084 | 651.0 | 573.2 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 24.70 | 148.73 | 11.90 | 329.53 | 0.3711 | 776.0 | 644.7 | |
| 0.00 | 1.93 | 0.00 | 1.04 | 27.59 | 148.13 | 11.31 | 334.57 | 0.4064 | 603.0 | 482.5 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 25.89 | 147.93 | 11.10 | 332.85 | 0.3813 | 994.0 | 836.6 | |
| 0.00 | 2.02 | 0.00 | 1.06 | 23.66 | 147.43 | 10.60 | 330.73 | 0.3462 | 898.0 | 743.2 | |
| 0.00 | 1.49 | 0.00 | 0.79 | 25.19 | 144.35 | 7.52 | 340.00 | 0.3476 | 846.0 | 511.2 | |
| 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. | |