SDO HMI 2011-10-17 17:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.40 | 44.74 | 10.99 | 26.73 | -15.04 | 2.49 | -27.15 | 128.00 | 0.5613 | -156.9 | -222.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.50 | 12.29 | 4.39 | 7.20 | -15.24 | 4.95 | -24.69 | 130.86 | 0.5351 | 926.3 | 636.4 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -14.67 | 4.10 | -25.54 | 129.08 | 0.5395 | 636.0 | 523.4 | |
| 0.00 | 0.87 | 0.00 | 0.51 | -14.48 | 4.09 | -25.55 | 128.79 | 0.5379 | 842.0 | 611.4 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -16.47 | 3.33 | -26.31 | 130.85 | 0.5640 | 682.0 | 533.6 | |
| 0.00 | 1.40 | 0.00 | 0.83 | -15.35 | 3.28 | -26.35 | 129.21 | 0.5546 | 706.0 | 479.9 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -16.07 | 2.24 | -27.40 | 129.17 | 0.5725 | -852.0 | -748.0 | |
| 0.00 | 1.31 | 0.00 | 0.79 | -16.08 | 2.06 | -27.57 | 129.00 | 0.5746 | -713.0 | -442.5 | |
| 0.00 | 1.40 | 0.00 | 0.83 | -14.29 | 2.18 | -27.46 | 126.53 | 0.5583 | -918.0 | -702.8 | |
| 0.00 | 1.40 | 0.00 | 0.83 | -14.30 | 1.93 | -27.70 | 126.30 | 0.5612 | -678.0 | -614.2 | |
| 0.70 | 8.98 | 0.42 | 5.44 | -15.81 | 1.65 | -27.99 | 128.21 | 0.5769 | -930.1 | -740.9 | |
| 1.13 | -10.00 | 0.69 | -10.00 | -15.65 | 1.60 | -28.04 | 127.94 | 0.5761 | -908.9 | 999999 | |
| 0.00 | 1.74 | 0.00 | 1.04 | -14.15 | 1.78 | -27.86 | 125.93 | 0.5618 | -818.0 | -756.7 | |
| 2.44 | -10.00 | 1.48 | -10.00 | -15.63 | 1.39 | -28.25 | 127.71 | 0.5783 | -704.1 | 999999 | |
| 6.63 | 12.56 | 4.01 | 7.60 | -14.42 | 0.73 | -28.91 | 125.34 | 0.5762 | -812.2 | -502.1 | |
| 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. | |