SDO HMI 2014-04-03 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.90 | 335.51 | 46.99 | 243.48 | 12.45 | 13.79 | -43.21 | 66.24 | 0.7327 | -787.7 | -281.3 | |
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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 | 0.59 | 3.84 | 15.75 | -41.25 | 77.08 | 0.6772 | 428.0 | 379.3 | |
| 57.26 | 320.05 | 41.36 | 231.77 | 12.47 | 14.06 | -42.94 | 66.09 | 0.7299 | -1153.5 | -324.2 | |
| 2.55 | -2.00 | 1.87 | -2.00 | 13.10 | 13.29 | -43.71 | 65.67 | 0.7410 | -314.8 | 999999 | |
| 5.09 | -2.00 | 3.76 | -2.00 | 12.63 | 12.84 | -44.16 | 66.47 | 0.7438 | -548.6 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.92 | 13.41 | 12.62 | -44.38 | 65.60 | 0.7494 | 204.0 | 153.6 | |
| 0.00 | 1.41 | 0.00 | 1.04 | 11.96 | 12.59 | -44.41 | 67.43 | 0.7437 | -250.0 | -210.1 | |
| 0.00 | 0.79 | 0.00 | 0.59 | 11.81 | 12.19 | -44.81 | 67.81 | 0.7473 | -214.0 | -166.7 | |
| 0.00 | 1.05 | 0.00 | 0.78 | 9.96 | 11.85 | -45.15 | 70.30 | 0.7439 | 638.0 | 496.0 | |
| 0.00 | 1.14 | 0.00 | 0.86 | 11.07 | 11.30 | -45.71 | 69.13 | 0.7541 | 637.0 | 560.0 | |
| 0.00 | 0.70 | 0.00 | 0.53 | 11.50 | 10.94 | -46.06 | 68.74 | 0.7594 | 687.0 | 651.0 | |
| 0.00 | 0.97 | 0.00 | 0.74 | 12.08 | 10.82 | -46.18 | 68.07 | 0.7629 | 498.0 | 452.1 | |
| 0.00 | 3.16 | 0.00 | 2.39 | 11.04 | 10.86 | -46.14 | 69.35 | 0.7586 | 635.0 | 522.2 | |
| 0.00 | 1.58 | 0.00 | 1.20 | 11.65 | 10.73 | -46.27 | 68.65 | 0.7622 | 785.0 | 628.1 | |
| 0.00 | 2.55 | 0.00 | 2.07 | 12.84 | 7.88 | -49.12 | 68.36 | 0.7953 | 634.0 | 495.3 | |
| 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. | |