SDO HMI 2014-04-14 11:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.05 | 266.19 | 22.43 | 139.05 | 12.27 | 262.93 | -3.41 | 10.17 | 0.3172 | -857.7 | -411.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.63 | 252.49 | 11.79 | 131.49 | 12.12 | 263.75 | -2.59 | 8.23 | 0.3098 | -1499.4 | -453.1 | |
| 20.42 | -1.00 | 10.64 | -1.00 | 12.09 | 263.35 | -2.99 | 9.49 | 0.3103 | -1384.3 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 18.71 | 262.62 | -3.71 | 8.46 | 0.4186 | -806.0 | -694.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 16.59 | 261.25 | -5.09 | 12.66 | 0.3893 | -737.0 | -561.1 | |
| 0.00 | 1.59 | 0.00 | 0.87 | 18.07 | 258.31 | -8.02 | 18.29 | 0.4246 | -794.0 | -633.5 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 18.11 | 255.71 | -10.62 | 23.58 | 0.4399 | -805.0 | -689.2 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 17.15 | 254.90 | -11.43 | 26.15 | 0.4316 | 748.0 | 549.7 | |
| 0.00 | 1.33 | 0.00 | 0.72 | 16.06 | 254.04 | -12.30 | 29.08 | 0.4228 | 812.0 | 717.5 | |
| 0.00 | 0.62 | 0.00 | 0.34 | 15.28 | 249.74 | -16.60 | 37.95 | 0.4499 | 523.0 | 458.4 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 16.12 | 249.61 | -16.73 | 37.00 | 0.4614 | 676.0 | 573.0 | |
| 0.00 | 1.24 | 0.00 | 0.69 | 12.05 | 246.25 | -20.09 | 48.40 | 0.4511 | 886.0 | 629.9 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 11.65 | 245.19 | -21.14 | 50.52 | 0.4596 | 758.0 | 629.3 | |
| 0.00 | 1.50 | 0.00 | 0.84 | 10.99 | 243.69 | -22.65 | 53.57 | 0.4717 | 827.0 | 642.5 | |
| 0.00 | 1.24 | 0.00 | 0.70 | 11.12 | 243.51 | -22.82 | 53.56 | 0.4751 | 789.0 | 553.3 | |
| 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. | |