SDO HMI 2014-10-08 23:06:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.93 | 0.00 | 10.43 | -18.70 | 75.77 | -3.89 | 171.89 | 0.4337 | 525.6 | 417.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.62 | -25.92 | 75.33 | -4.33 | 172.74 | 0.5394 | 506.0 | 393.8 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -25.73 | 63.67 | -16.00 | 154.76 | 0.5844 | -673.0 | -566.1 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -21.14 | 82.15 | 2.48 | 185.01 | 0.4646 | 775.0 | 489.1 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -20.41 | 74.23 | -5.43 | 168.83 | 0.4597 | 501.0 | 343.9 | |
| 0.00 | 1.40 | 0.00 | 0.79 | -20.68 | 72.20 | -7.46 | 164.98 | 0.4709 | 741.0 | 647.1 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -19.92 | 74.29 | -5.38 | 168.72 | 0.4521 | 691.0 | 558.5 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -18.79 | 79.13 | -0.54 | 178.80 | 0.4261 | 822.0 | 642.2 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -19.67 | 72.78 | -6.89 | 165.53 | 0.4536 | -774.0 | -627.4 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -16.93 | 77.31 | -2.35 | 174.31 | 0.3982 | 873.0 | 678.3 | |
| 0.00 | 1.49 | 0.00 | 0.80 | -16.19 | 80.42 | 0.76 | 181.90 | 0.3845 | 908.0 | 724.7 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -16.89 | 77.05 | -2.62 | 173.67 | 0.3979 | 663.0 | 543.1 | |
| 0.00 | 1.75 | 0.00 | 0.94 | -16.74 | 77.44 | -2.23 | 174.57 | 0.3949 | 690.0 | 558.2 | |
| 0.00 | 1.84 | 0.00 | 0.98 | -15.13 | 80.94 | 1.28 | 183.38 | 0.3677 | 877.0 | 639.6 | |
| 0.00 | 1.84 | 0.00 | 0.99 | -14.26 | 70.23 | -9.44 | 155.58 | 0.3860 | 758.0 | 585.7 | |
| 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. | |