SDO HMI 2014-03-24 19:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.45 | 0.00 | 9.41 | -11.30 | 133.82 | -45.20 | 98.93 | 0.7071 | 541.3 | 450.6 | |
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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 | 1.14 | 0.00 | 0.74 | -7.11 | 138.29 | -40.73 | 92.88 | 0.6506 | 706.0 | 602.4 | |
| 0.00 | 1.22 | 0.00 | 0.80 | -7.15 | 138.01 | -41.01 | 92.96 | 0.6543 | 628.0 | 492.7 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -10.27 | 135.68 | -43.34 | 97.68 | 0.6838 | 639.0 | 561.6 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -9.07 | 135.83 | -43.19 | 95.93 | 0.6818 | 214.0 | 234.5 | |
| 0.00 | 0.96 | 0.00 | 0.65 | -10.25 | 135.52 | -43.50 | 97.65 | 0.6858 | 585.0 | 497.3 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -6.48 | 135.67 | -43.35 | 92.12 | 0.6848 | 491.0 | 318.4 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -15.55 | 131.77 | -47.25 | 104.85 | 0.7342 | 640.0 | 530.5 | |
| 0.00 | 0.52 | 0.00 | 0.38 | -14.96 | 131.72 | -47.30 | 104.05 | 0.7343 | 585.0 | 535.5 | |
| 0.00 | 2.44 | 0.00 | 1.78 | -14.66 | 131.71 | -47.31 | 103.63 | 0.7340 | 654.0 | 464.7 | |
| 0.00 | 1.66 | 0.00 | 1.23 | -15.15 | 130.69 | -48.33 | 104.19 | 0.7461 | 382.0 | 365.9 | |
| 0.00 | 0.70 | 0.00 | 0.50 | -9.08 | 132.04 | -46.98 | 96.00 | 0.7282 | 426.0 | 359.2 | |
| 0.00 | 0.61 | 0.00 | 0.44 | -8.06 | 131.68 | -47.34 | 94.60 | 0.7328 | 546.0 | 503.1 | |
| 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. | |