SDO HMI 2014-10-03 12:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.56 | 39.60 | 3.98 | 21.19 | -11.30 | 139.19 | -12.57 | 144.95 | 0.3737 | 120.9 | 80.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.10 | 16.54 | 2.69 | 8.73 | -9.90 | 140.36 | -11.39 | 145.36 | 0.3439 | 1054.8 | 710.8 | |
| 0.88 | 4.49 | 0.46 | 2.36 | -9.31 | 140.29 | -11.47 | 144.18 | 0.3367 | 1122.8 | 907.4 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -16.88 | 139.92 | -11.84 | 153.62 | 0.4438 | 604.0 | 481.1 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -11.41 | 140.18 | -11.58 | 147.33 | 0.3661 | 812.0 | 610.8 | |
| 1.58 | -1.00 | 0.83 | -1.00 | -9.72 | 140.18 | -11.57 | 144.63 | 0.3431 | 1114.1 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -14.60 | 138.81 | -12.94 | 148.86 | 0.4209 | -572.0 | -544.0 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -13.49 | 138.28 | -13.48 | 146.34 | 0.4107 | -779.0 | -606.8 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -8.73 | 138.48 | -13.28 | 139.01 | 0.3477 | 801.0 | 646.6 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -14.14 | 138.11 | -13.64 | 146.89 | 0.4206 | -831.0 | -659.4 | |
| 0.00 | 5.72 | 0.00 | 3.10 | -12.99 | 138.15 | -13.61 | 145.37 | 0.4052 | -499.0 | -702.8 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -14.60 | 137.73 | -14.03 | 146.78 | 0.4299 | -809.0 | -615.6 | |
| 0.00 | 2.11 | 0.00 | 1.15 | -12.64 | 136.93 | -14.82 | 142.53 | 0.4121 | -650.0 | -480.5 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -11.82 | 136.82 | -14.94 | 141.05 | 0.4030 | -712.0 | -596.5 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -10.63 | 133.61 | -18.15 | 133.50 | 0.4239 | -835.0 | -723.7 | |
| 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. | |