SDO HMI 2014-01-15 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 |
| 9.77 | 37.03 | 6.28 | 23.16 | 16.23 | 27.84 | 31.48 | 304.67 | 0.6108 | 42.4 | 44.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.63 | 10.88 | 4.29 | 7.04 | 15.90 | 31.11 | 34.76 | 301.53 | 0.6456 | -839.4 | -590.0 | |
| 2.04 | 3.74 | 1.31 | 2.40 | 16.03 | 30.47 | 34.11 | 302.16 | 0.6391 | -755.7 | -546.7 | |
| 0.68 | 5.35 | 0.43 | 3.42 | 15.94 | 30.01 | 33.65 | 302.38 | 0.6333 | -835.0 | -757.0 | |
| 0.00 | 1.61 | 0.00 | 0.99 | 15.67 | 26.63 | 30.28 | 304.68 | 0.5925 | 767.0 | 637.9 | |
| 0.00 | 1.61 | 0.00 | 0.98 | 15.94 | 25.33 | 28.98 | 306.20 | 0.5796 | -813.0 | -572.6 | |
| 0.00 | 0.93 | 0.00 | 0.57 | 17.25 | 25.05 | 28.70 | 308.33 | 0.5870 | 461.0 | 394.5 | |
| 0.00 | 2.04 | 0.00 | 1.24 | 17.33 | 24.65 | 28.29 | 308.83 | 0.5831 | 909.0 | 706.0 | |
| 0.00 | 1.87 | 0.00 | 1.13 | 17.04 | 24.56 | 28.21 | 308.50 | 0.5798 | 836.0 | 702.6 | |
| 0.00 | 0.85 | 0.00 | 0.51 | 16.11 | 24.27 | 27.92 | 307.45 | 0.5689 | 519.0 | 515.5 | |
| 0.00 | 2.38 | 0.00 | 1.43 | 16.11 | 24.10 | 27.75 | 307.61 | 0.5669 | 676.0 | 625.0 | |
| 0.42 | 1.87 | 0.25 | 1.11 | 15.86 | 23.30 | 26.95 | 308.03 | 0.5557 | 957.6 | 829.2 | |
| 0.00 | 1.10 | 0.00 | 0.67 | 18.27 | 23.55 | 27.20 | 311.22 | 0.5792 | 498.0 | 417.9 | |
| 0.00 | 1.95 | 0.00 | 1.16 | 16.28 | 22.81 | 26.46 | 309.15 | 0.5537 | 883.0 | 729.3 | |
| 0.00 | 0.85 | 0.00 | 0.51 | 17.99 | 21.97 | 25.62 | 312.48 | 0.5598 | 627.0 | 527.0 | |
| 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. | |