SDO HMI 2011-10-05 03:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.58 | 370.42 | 42.19 | 245.45 | 23.23 | 156.03 | -39.60 | 62.01 | 0.6656 | -838.2 | -307.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.65 | 26.69 | 156.63 | -39.00 | 56.86 | 0.6739 | -771.0 | -704.9 | |
| 0.00 | 1.49 | 0.00 | 1.00 | 25.51 | 156.28 | -39.35 | 58.67 | 0.6722 | -147.0 | -233.7 | |
| 14.51 | 296.46 | 9.50 | 195.00 | 22.66 | 156.64 | -38.99 | 62.58 | 0.6564 | -1136.4 | -362.4 | |
| 27.96 | -3.00 | 18.42 | -3.00 | 23.18 | 156.34 | -39.29 | 61.96 | 0.6619 | -1115.1 | 999999 | |
| 1.06 | -3.00 | 0.69 | -3.00 | 22.27 | 156.40 | -39.23 | 63.26 | 0.6577 | -776.2 | 999999 | |
| 1.41 | -3.00 | 0.93 | -3.00 | 22.47 | 156.16 | -39.47 | 63.06 | 0.6612 | -570.6 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.65 | 24.86 | 155.24 | -40.39 | 60.04 | 0.6810 | -129.0 | -91.0 | |
| 17.23 | 62.51 | 11.63 | 42.33 | 24.13 | 154.96 | -40.67 | 61.17 | 0.6813 | -913.4 | -108.5 | |
| 0.00 | 0.79 | 0.00 | 0.53 | 21.58 | 155.07 | -40.56 | 64.77 | 0.6708 | -611.0 | -491.0 | |
| 0.00 | 1.06 | 0.00 | 0.75 | 25.17 | 151.61 | -44.02 | 61.02 | 0.7213 | 501.0 | 407.7 | |
| 1.41 | 2.29 | 1.02 | 1.66 | 24.73 | 150.46 | -45.17 | 61.99 | 0.7320 | 589.8 | 429.4 | |
| 0.00 | 1.85 | 0.00 | 1.39 | 26.33 | 148.70 | -46.93 | 60.46 | 0.7548 | 628.0 | 554.1 | |
| 0.00 | 1.06 | 0.00 | 0.76 | 22.43 | 150.36 | -45.27 | 65.09 | 0.7264 | 398.0 | 311.2 | |
| 0.00 | 0.97 | 0.00 | 0.73 | 25.10 | 147.87 | -47.76 | 62.29 | 0.7596 | 487.0 | 431.0 | |
| 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. | |