SDO HMI 2014-04-07 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.77 | 420.35 | 42.03 | 227.27 | 12.74 | 13.46 | 14.17 | 323.34 | 0.4017 | -1072.4 | -389.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.85 | 0.00 | 0.99 | 10.39 | 13.59 | 14.31 | 319.20 | 0.3736 | 822.0 | 666.7 | |
| 0.00 | 0.26 | 0.00 | 0.14 | 10.58 | 13.51 | 14.22 | 319.69 | 0.3750 | 592.0 | 617.7 | |
| 74.42 | 401.69 | 40.22 | 217.22 | 12.69 | 13.56 | 14.27 | 323.06 | 0.4019 | -1453.4 | -414.6 | |
| 3.35 | -3.00 | 1.81 | -3.00 | 13.31 | 13.18 | 13.90 | 324.72 | 0.4064 | -1020.2 | 999999 | |
| 0.00 | 2.82 | 0.00 | 1.54 | 14.80 | 12.74 | 13.45 | 327.65 | 0.4220 | 790.0 | 689.8 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 14.67 | 12.54 | 13.25 | 327.86 | 0.4185 | 935.0 | 695.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 12.30 | 11.80 | 12.51 | 326.02 | 0.3804 | -675.0 | -481.2 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 14.78 | 11.84 | 12.56 | 329.37 | 0.4143 | -599.0 | -500.0 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 11.79 | 11.56 | 12.27 | 325.77 | 0.3714 | -752.0 | -603.8 | |
| 0.00 | 2.38 | 0.00 | 1.29 | 14.68 | 11.61 | 12.33 | 329.70 | 0.4111 | -679.0 | -556.2 | |
| 0.00 | 2.55 | 0.00 | 1.38 | 14.55 | 11.35 | 12.07 | 330.06 | 0.4071 | -845.0 | -757.3 | |
| 0.00 | 1.59 | 0.00 | 0.84 | 11.33 | 11.07 | 11.78 | 326.15 | 0.3609 | 797.0 | 633.8 | |
| 0.00 | 0.53 | 0.00 | 0.29 | 14.70 | 11.14 | 11.85 | 330.69 | 0.4076 | -617.0 | -634.0 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 14.51 | 9.39 | 10.10 | 334.20 | 0.3919 | 738.0 | 480.8 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 9.78 | 8.22 | 8.93 | 330.76 | 0.3146 | 783.0 | 556.2 | |
| 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. | |