SDO HMI 2014-01-13 16:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 96.02 | 462.01 | 49.31 | 237.37 | -16.48 | 13.08 | -9.60 | 142.89 | 0.2661 | 1043.8 | 388.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.14 | 281.87 | 30.33 | 144.49 | -16.60 | 13.78 | -8.91 | 145.05 | 0.2603 | 1410.9 | 468.0 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -16.32 | 12.76 | -9.93 | 141.47 | 0.2668 | 924.0 | 696.6 | |
| 0.00 | 2.21 | 0.00 | 1.13 | -15.74 | 12.76 | -9.93 | 140.03 | 0.2595 | 847.0 | 584.0 | |
| 0.00 | 2.55 | 0.00 | 1.31 | -15.32 | 12.69 | -10.00 | 138.72 | 0.2550 | 1056.0 | 800.5 | |
| 5.10 | 164.69 | 2.63 | 84.82 | -16.73 | 12.52 | -10.17 | 141.82 | 0.2747 | 1105.8 | 310.4 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -14.75 | 12.34 | -10.34 | 136.19 | 0.2520 | -840.0 | -506.2 | |
| 31.78 | -5.00 | 16.35 | -5.00 | -16.28 | 12.23 | -10.45 | 139.95 | 0.2719 | 1267.0 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -16.87 | 7.87 | -14.81 | 131.76 | 0.3295 | -664.0 | -492.1 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -15.52 | 6.90 | -15.79 | 126.76 | 0.3287 | -866.0 | -704.6 | |
| 0.00 | 1.10 | 0.00 | 0.58 | -15.04 | 6.84 | -15.84 | 125.43 | 0.3250 | -883.0 | -693.1 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -16.02 | 6.22 | -16.47 | 126.90 | 0.3422 | -798.0 | -661.3 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -18.34 | 4.73 | -17.95 | 129.90 | 0.3831 | -798.0 | -692.2 | |
| 0.00 | 0.76 | 0.00 | 0.41 | -18.10 | 3.55 | -19.14 | 127.72 | 0.3957 | -723.0 | -652.2 | |
| 0.00 | 1.10 | 0.00 | 0.58 | -12.21 | 3.50 | -19.19 | 113.58 | 0.3521 | -721.0 | -610.5 | |
| 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. | |