SDO HMI 2014-05-16 23:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.87 | 54.28 | 9.10 | 27.65 | -15.70 | 194.22 | -2.59 | 169.11 | 0.2346 | 328.8 | 350.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.03 | 15.54 | 2.57 | 7.94 | -16.65 | 195.21 | -1.60 | 173.75 | 0.2474 | 1046.8 | 830.8 | |
| 3.50 | 6.65 | 1.78 | 3.39 | -15.87 | 195.16 | -1.66 | 173.15 | 0.2343 | 1103.7 | 749.2 | |
| 0.00 | 0.45 | 0.00 | 0.23 | -16.96 | 195.05 | -1.76 | 173.28 | 0.2529 | 544.0 | 419.2 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -15.87 | 194.94 | -1.88 | 172.24 | 0.2347 | 158.0 | 149.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -16.58 | 194.71 | -2.11 | 171.77 | 0.2474 | 873.0 | 674.9 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -12.86 | 194.75 | -2.07 | 168.96 | 0.1845 | -774.0 | -567.7 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -12.55 | 194.50 | -2.31 | 167.31 | 0.1802 | -946.0 | -732.7 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -15.31 | 194.41 | -2.41 | 169.66 | 0.2267 | 689.0 | 580.9 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -15.09 | 193.81 | -3.00 | 166.96 | 0.2251 | 798.0 | 701.6 | |
| 3.32 | 16.17 | 1.69 | 8.23 | -15.40 | 193.59 | -3.23 | 166.36 | 0.2311 | 253.2 | 84.2 | |
| 2.07 | -10.00 | 1.05 | -10.00 | -15.24 | 193.43 | -3.38 | 165.56 | 0.2292 | 1087.3 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -15.86 | 193.26 | -3.55 | 165.57 | 0.2401 | -583.0 | -404.1 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -14.93 | 192.87 | -3.94 | 162.88 | 0.2267 | 930.0 | 753.5 | |
| 3.95 | 5.75 | 2.01 | 2.93 | -15.33 | 192.42 | -4.39 | 161.64 | 0.2355 | -976.5 | -702.7 | |
| 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. | |