SDO HMI 2014-11-04 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.39 | 26.60 | 3.52 | 14.49 | -17.62 | 98.89 | 10.30 | 204.56 | 0.4152 | -120.7 | -44.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.39 | 9.07 | 3.52 | 4.99 | -16.71 | 104.08 | 15.49 | 216.04 | 0.4367 | 1001.8 | 753.5 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -15.28 | 103.71 | 15.13 | 217.48 | 0.4154 | -817.0 | -677.3 | |
| 0.00 | 2.85 | 0.00 | 1.55 | -16.84 | 100.98 | 12.40 | 210.09 | 0.4116 | 627.0 | 536.1 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -16.77 | 100.53 | 11.95 | 209.28 | 0.4071 | 1139.0 | 850.2 | |
| 0.00 | 1.81 | 0.00 | 0.98 | -17.66 | 98.40 | 9.82 | 203.78 | 0.4045 | 803.0 | 627.1 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.11 | 94.98 | 6.39 | 196.46 | 0.3772 | -864.0 | -669.2 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.65 | 94.62 | 6.03 | 195.19 | 0.3840 | -760.0 | -577.4 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -17.55 | 94.36 | 5.78 | 194.65 | 0.3814 | -856.0 | -677.6 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -18.00 | 93.88 | 5.29 | 193.18 | 0.3865 | -861.0 | -759.9 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -19.12 | 93.91 | 5.33 | 192.58 | 0.4043 | -668.0 | -558.2 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -17.99 | 93.69 | 5.10 | 192.72 | 0.3858 | -988.0 | -902.8 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -18.18 | 93.44 | 4.86 | 192.02 | 0.3880 | -855.0 | -603.4 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -20.99 | 90.72 | 2.13 | 184.70 | 0.4262 | -668.0 | -440.1 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -22.74 | 89.90 | 1.32 | 182.70 | 0.4528 | -752.0 | -592.3 | |
| 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. | |