SDO HMI 2014-04-07 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.38 | 0.00 | 10.06 | -17.82 | 350.84 | -11.18 | 139.17 | 0.2975 | -627.8 | -604.0 | |
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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 |
| 0.00 | 0.88 | 0.00 | 0.47 | -22.83 | 17.30 | 15.28 | 219.96 | 0.3798 | 824.0 | 710.2 | |
| 0.00 | 2.03 | 0.00 | 1.03 | -17.81 | 356.12 | -5.91 | 154.13 | 0.2255 | -905.0 | -607.5 | |
| 0.00 | 1.85 | 0.00 | 0.94 | -18.23 | 355.53 | -6.49 | 152.84 | 0.2363 | -908.0 | -802.6 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -11.33 | 354.97 | -7.05 | 126.92 | 0.1512 | -776.0 | -592.6 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -18.10 | 353.08 | -8.94 | 144.58 | 0.2560 | -791.0 | -619.1 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -22.16 | 351.85 | -10.17 | 149.43 | 0.3229 | -725.0 | -562.8 | |
| 0.00 | 1.94 | 0.00 | 0.99 | -14.61 | 349.46 | -12.56 | 125.28 | 0.2590 | -886.0 | -666.7 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -15.51 | 348.96 | -13.07 | 127.08 | 0.2743 | -700.0 | -628.9 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -23.02 | 348.12 | -13.90 | 142.90 | 0.3683 | -765.0 | -537.5 | |
| 0.00 | 6.17 | 0.00 | 3.25 | -17.66 | 345.02 | -17.00 | 126.12 | 0.3465 | -554.0 | -745.8 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -17.71 | 344.62 | -17.40 | 125.65 | 0.3522 | -720.0 | -543.2 | |
| 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. | |