SDO HMI 2014-04-08 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.40 | 90.44 | 12.77 | 47.41 | 10.41 | 359.92 | 8.90 | 332.49 | 0.3274 | -183.6 | -344.1 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.29 | 33.29 | 1.21 | 17.63 | 10.21 | 4.01 | 12.98 | 321.59 | 0.3575 | -855.7 | -846.5 | |
| 2.64 | -1.00 | 1.40 | -1.00 | 10.02 | 3.84 | 12.82 | 321.61 | 0.3534 | -1073.9 | 999999 | |
| 5.20 | -1.00 | 2.75 | -1.00 | 10.37 | 3.79 | 12.77 | 322.32 | 0.3573 | -876.2 | 999999 | |
| 1.32 | -1.00 | 0.70 | -1.00 | 10.14 | 3.69 | 12.67 | 322.16 | 0.3534 | -1192.0 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 8.57 | 3.07 | 12.05 | 320.64 | 0.3270 | -835.0 | -606.8 | |
| 0.00 | 1.76 | 0.00 | 0.92 | 8.60 | 2.89 | 11.86 | 321.13 | 0.3254 | -1079.0 | -845.3 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 10.22 | 2.82 | 11.80 | 324.25 | 0.3459 | -715.0 | -587.9 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 12.16 | 2.47 | 11.44 | 328.13 | 0.3689 | -689.0 | -558.5 | |
| 0.00 | 5.55 | 0.00 | 2.94 | 11.80 | 1.82 | 10.80 | 329.07 | 0.3585 | -950.0 | -766.4 | |
| 9.34 | 41.92 | 4.84 | 21.75 | 10.09 | 356.89 | 5.87 | 340.16 | 0.2980 | 979.0 | 6.2 | |
| 3.61 | -10.00 | 1.87 | -10.00 | 10.25 | 356.34 | 5.32 | 342.05 | 0.2974 | -980.5 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 9.24 | 356.14 | 5.12 | 341.61 | 0.2804 | 755.0 | 596.9 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 13.55 | 355.11 | 4.09 | 348.37 | 0.3453 | 736.0 | 583.0 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 14.22 | 355.00 | 3.98 | 349.06 | 0.3557 | 871.0 | 655.0 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 14.45 | 354.97 | 3.95 | 349.25 | 0.3592 | 786.0 | 662.7 | |
| 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. | |