SDO HMI 2014-04-23 10:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.58 | 382.09 | 34.99 | 216.93 | 17.80 | 166.64 | 18.61 | 321.50 | 0.4900 | -828.1 | -320.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.58 | 359.87 | 34.99 | 204.55 | 17.78 | 166.88 | 18.85 | 321.09 | 0.4919 | -1351.7 | -386.7 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 17.28 | 165.39 | 17.37 | 322.67 | 0.4720 | -870.0 | -674.6 | |
| 0.00 | 1.33 | 0.00 | 0.75 | 17.67 | 165.43 | 17.41 | 323.13 | 0.4771 | -358.0 | -307.5 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 18.14 | 163.20 | 15.18 | 327.37 | 0.4633 | 744.0 | 605.8 | |
| 0.00 | 1.33 | 0.00 | 0.74 | 18.30 | 162.95 | 14.93 | 327.99 | 0.4633 | 822.0 | 639.2 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 19.19 | 162.93 | 14.91 | 329.06 | 0.4746 | 611.0 | 533.8 | |
| 0.00 | 7.11 | 0.00 | 3.96 | 18.03 | 162.76 | 14.74 | 327.99 | 0.4583 | 1087.0 | 846.6 | |
| 0.00 | 1.24 | 0.00 | 0.70 | 18.95 | 162.81 | 14.79 | 329.00 | 0.4706 | 679.0 | 587.1 | |
| 0.00 | 1.42 | 0.00 | 0.80 | 18.88 | 162.61 | 14.58 | 329.27 | 0.4681 | 800.0 | 615.8 | |
| 0.00 | 1.33 | 0.00 | 0.75 | 19.88 | 162.63 | 14.61 | 330.34 | 0.4813 | 732.0 | 542.8 | |
| 0.00 | 1.16 | 0.00 | 0.64 | 18.28 | 161.96 | 13.94 | 329.69 | 0.4551 | 877.0 | 742.8 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 17.42 | 161.50 | 13.48 | 329.50 | 0.4400 | 929.0 | 754.9 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 17.12 | 161.35 | 13.33 | 329.42 | 0.4349 | 559.0 | 455.5 | |
| 0.00 | 1.87 | 0.00 | 1.02 | 17.11 | 160.41 | 12.39 | 331.19 | 0.4273 | 942.0 | 747.8 | |
| 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. | |