SDO HMI 2014-11-04 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.78 | 38.08 | 6.48 | 19.66 | 5.65 | 70.78 | -15.59 | 82.82 | 0.2701 | -133.8 | 124.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.44 | 7.59 | 75.35 | -11.03 | 71.49 | 0.2009 | -815.0 | -606.5 | |
| 12.78 | 18.23 | 6.48 | 9.24 | 5.85 | 74.04 | -12.33 | 81.06 | 0.2161 | -1173.7 | -820.7 | |
| 0.00 | 4.06 | 0.00 | 2.06 | 5.28 | 73.69 | -12.69 | 83.84 | 0.2210 | -598.0 | -448.8 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 5.81 | 73.65 | -12.73 | 81.46 | 0.2227 | -667.0 | -538.4 | |
| 0.00 | 1.47 | 0.00 | 0.77 | 5.61 | 67.16 | -19.22 | 84.51 | 0.3307 | 657.0 | 503.5 | |
| 0.00 | 4.92 | 0.00 | 2.60 | 4.63 | 66.11 | -20.27 | 87.52 | 0.3472 | 902.0 | 885.2 | |
| 0.00 | 1.47 | 0.00 | 0.78 | 5.01 | 65.84 | -20.54 | 86.45 | 0.3517 | 1006.0 | 809.9 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 6.22 | 65.13 | -21.25 | 83.20 | 0.3645 | 888.0 | 747.0 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 6.01 | 65.07 | -21.31 | 83.79 | 0.3651 | 975.0 | 778.9 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 5.94 | 64.88 | -21.50 | 84.00 | 0.3681 | 833.0 | 683.1 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 6.02 | 64.62 | -21.76 | 83.83 | 0.3724 | 630.0 | 533.5 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 5.95 | 64.01 | -22.37 | 84.14 | 0.3822 | 681.0 | 434.8 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 6.10 | 64.00 | -22.38 | 83.75 | 0.3825 | 641.0 | 468.7 | |
| 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. | |