SDO HMI 2014-05-17 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.82 | 186.87 | 32.63 | 95.44 | -16.08 | 194.33 | 3.56 | 193.92 | 0.2454 | 169.3 | 196.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.66 | 76.85 | 2.90 | 39.42 | -16.54 | 195.69 | 4.92 | 198.58 | 0.2589 | 1226.0 | 716.0 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -15.63 | 195.66 | 4.89 | 199.73 | 0.2444 | 918.0 | 674.5 | |
| 24.36 | -1.00 | 12.51 | -1.00 | -16.95 | 195.60 | 4.83 | 197.77 | 0.2650 | 1125.5 | 999999 | |
| 3.15 | -1.00 | 1.61 | -1.00 | -16.13 | 195.49 | 4.72 | 198.39 | 0.2514 | 1153.1 | 999999 | |
| 0.00 | 2.43 | 0.00 | 1.24 | -16.85 | 194.96 | 4.19 | 195.66 | 0.2604 | 796.0 | 646.4 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -16.54 | 194.70 | 3.93 | 195.06 | 0.2542 | 668.0 | 432.8 | |
| 0.00 | 2.07 | 0.00 | 1.06 | -16.82 | 194.55 | 3.78 | 194.21 | 0.2581 | 1024.0 | 679.0 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -14.95 | 194.23 | 3.46 | 195.03 | 0.2261 | 922.0 | 743.0 | |
| 0.00 | 0.72 | 0.00 | 0.37 | -15.89 | 194.22 | 3.45 | 193.92 | 0.2414 | 694.0 | 388.1 | |
| 5.12 | 97.43 | 2.61 | 49.60 | -15.42 | 193.77 | 3.00 | 192.61 | 0.2319 | -1010.4 | -160.3 | |
| 20.22 | -10.00 | 10.30 | -10.00 | -15.48 | 193.27 | 2.49 | 190.50 | 0.2312 | -1237.0 | 999999 | |
| 2.97 | -10.00 | 1.51 | -10.00 | -15.86 | 193.24 | 2.47 | 190.09 | 0.2374 | -968.4 | 999999 | |
| 2.34 | 4.22 | 1.19 | 2.15 | -15.30 | 192.57 | 1.80 | 187.74 | 0.2262 | -952.8 | -713.7 | |
| 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. | |