SDO HMI 2014-09-06 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.32 | 84.48 | 19.01 | 45.34 | -14.95 | 149.02 | 4.16 | 190.67 | 0.3856 | -243.7 | 167.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.63 | -16.49 | 149.89 | 5.04 | 191.82 | 0.4125 | -844.0 | -631.1 | |
| 10.08 | 44.52 | 5.35 | 23.63 | -13.29 | 149.42 | 4.56 | 192.45 | 0.3603 | 1145.6 | 701.6 | |
| 0.00 | 1.34 | 0.00 | 0.71 | -12.81 | 149.41 | 4.55 | 192.73 | 0.3526 | 255.0 | 259.3 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -16.19 | 149.45 | 4.59 | 190.94 | 0.4064 | -814.0 | -599.7 | |
| 7.76 | 29.26 | 4.22 | 15.89 | -16.65 | 149.27 | 4.41 | 190.31 | 0.4131 | -959.3 | -824.2 | |
| 4.46 | -2.00 | 2.37 | -2.00 | -13.64 | 149.11 | 4.25 | 191.44 | 0.3649 | 863.2 | 999999 | |
| 0.80 | -2.00 | 0.43 | -2.00 | -13.35 | 149.01 | 4.16 | 191.35 | 0.3600 | 1005.3 | 999999 | |
| 12.22 | -5.00 | 6.64 | -5.00 | -16.58 | 148.89 | 4.03 | 189.47 | 0.4109 | -1132.5 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.65 | -19.86 | 148.38 | 3.52 | 187.23 | 0.4609 | -680.0 | -505.8 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -16.67 | 148.29 | 3.43 | 188.05 | 0.4110 | -805.0 | -654.5 | |
| 0.00 | 1.25 | 0.00 | 0.67 | -16.11 | 147.77 | 2.91 | 187.03 | 0.4009 | -985.0 | -863.5 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -14.83 | 147.76 | 2.90 | 187.41 | 0.3804 | -899.0 | -752.3 | |
| 0.00 | 1.78 | 0.00 | 0.96 | -15.38 | 147.20 | 2.34 | 185.85 | 0.3883 | -929.0 | -659.8 | |
| 0.00 | 1.34 | 0.00 | 0.76 | -21.93 | 144.35 | -0.51 | 179.04 | 0.4895 | 588.0 | 564.5 | |
| 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. | |