SDO HMI 2014-11-01 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.22 | 33.40 | 7.27 | 30.16 | 6.20 | 69.53 | -56.96 | 85.42 | 0.8378 | -190.5 | -227.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.71 | 16.52 | 4.96 | 14.34 | 6.17 | 71.03 | -55.46 | 85.50 | 0.8237 | -818.8 | -601.1 | |
| 1.47 | 2.86 | 1.29 | 2.50 | 6.69 | 70.78 | -55.71 | 84.85 | 0.8261 | -538.6 | -457.9 | |
| 0.00 | 1.73 | 0.00 | 1.52 | 6.32 | 70.57 | -55.92 | 85.30 | 0.8281 | -234.0 | -210.6 | |
| 0.00 | 0.78 | 0.00 | 0.71 | 6.71 | 69.08 | -57.41 | 84.81 | 0.8424 | -468.0 | -409.1 | |
| 0.00 | 1.56 | 0.00 | 1.42 | 6.35 | 69.09 | -57.40 | 85.24 | 0.8423 | -352.0 | -334.9 | |
| 0.00 | 1.12 | 0.00 | 1.03 | 6.10 | 68.96 | -57.53 | 85.53 | 0.8436 | -350.0 | -323.5 | |
| 0.00 | 1.12 | 0.00 | 1.04 | 6.47 | 68.73 | -57.76 | 85.08 | 0.8457 | -319.0 | -244.2 | |
| 0.00 | 0.78 | 0.00 | 0.76 | 6.23 | 66.85 | -59.64 | 85.31 | 0.8627 | 302.0 | 400.3 | |
| 1.04 | 2.77 | 1.02 | 2.71 | 6.25 | 66.55 | -59.94 | 85.29 | 0.8653 | 545.2 | 445.4 | |
| 0.00 | 0.43 | 0.00 | 0.43 | 5.97 | 66.48 | -60.01 | 85.61 | 0.8660 | 569.0 | 544.8 | |
| 0.00 | 0.87 | 0.00 | 0.86 | 5.48 | 66.26 | -60.22 | 86.17 | 0.8680 | 575.0 | 487.5 | |
| 0.00 | 1.56 | 0.00 | 1.55 | 5.74 | 66.16 | -60.33 | 85.86 | 0.8688 | 472.0 | 408.9 | |
| 0.00 | 1.04 | 0.00 | 1.03 | 5.94 | 66.06 | -60.43 | 85.63 | 0.8696 | 324.0 | 271.8 | |
| 0.00 | 0.26 | 0.00 | 0.26 | 5.57 | 65.88 | -60.61 | 86.05 | 0.8712 | 201.0 | 186.3 | |
| 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. | |