SDO HMI 2014-03-02 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.52 | 29.02 | 0.28 | 15.84 | 7.62 | 135.53 | 19.43 | 307.70 | 0.4168 | 129.6 | 283.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.66 | 10.33 | 143.19 | 27.08 | 302.75 | 0.5347 | -547.0 | -473.8 | |
| 0.00 | 1.21 | 0.00 | 0.71 | 10.25 | 142.98 | 26.87 | 302.84 | 0.5315 | -735.0 | -495.9 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 5.22 | 141.46 | 25.36 | 295.52 | 0.4745 | -599.0 | -517.4 | |
| 0.00 | 2.25 | 0.00 | 1.26 | 5.20 | 141.10 | 24.99 | 295.82 | 0.4694 | -784.0 | -653.1 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 4.38 | 139.33 | 23.23 | 295.92 | 0.4391 | -825.0 | -726.8 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 7.05 | 136.38 | 20.28 | 304.78 | 0.4206 | 793.0 | 657.8 | |
| 0.00 | 3.37 | 0.00 | 1.84 | 7.50 | 136.28 | 20.18 | 305.81 | 0.4235 | 761.0 | 630.2 | |
| 0.00 | 1.64 | 0.00 | 0.90 | 8.55 | 135.57 | 19.46 | 308.79 | 0.4246 | -968.0 | -763.1 | |
| 0.00 | 1.99 | 0.00 | 1.07 | 6.85 | 134.50 | 18.40 | 307.08 | 0.3945 | 776.0 | 638.7 | |
| 0.00 | 1.64 | 0.00 | 0.88 | 7.77 | 133.88 | 17.78 | 309.90 | 0.3961 | 397.0 | 424.9 | |
| 0.52 | 7.25 | 0.28 | 3.90 | 8.21 | 133.15 | 17.04 | 311.95 | 0.3917 | 995.3 | 768.6 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 8.66 | 131.13 | 15.03 | 316.44 | 0.3737 | 655.0 | 511.9 | |
| 0.00 | 2.68 | 0.00 | 1.42 | 8.12 | 130.71 | 14.60 | 316.25 | 0.3626 | 744.0 | 784.7 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 7.28 | 130.46 | 14.36 | 315.10 | 0.3500 | 909.0 | 683.9 | |
| 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. | |