SDO HMI 2014-04-07 04:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 22.74 | 0.39 | 11.31 | -8.64 | 6.85 | 4.28 | 236.92 | 0.0995 | 25.7 | 1.0 | |
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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 | 1.50 | 0.00 | 0.75 | -7.87 | 11.68 | 9.10 | 258.96 | 0.1604 | 925.0 | 685.3 | |
| 0.00 | 2.55 | 0.00 | 1.28 | -8.78 | 10.62 | 8.05 | 251.52 | 0.1466 | 883.0 | 621.7 | |
| 0.00 | 1.94 | 0.00 | 0.97 | -9.20 | 10.60 | 8.03 | 248.76 | 0.1486 | 901.0 | 670.7 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -9.30 | 10.42 | 7.85 | 247.74 | 0.1463 | 1004.0 | 850.5 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -9.18 | 10.08 | 7.51 | 247.64 | 0.1401 | 899.0 | 738.2 | |
| 0.00 | 1.41 | 0.00 | 0.70 | -10.40 | 8.26 | 5.69 | 232.83 | 0.1230 | 869.0 | 703.2 | |
| 0.00 | 0.79 | 0.00 | 0.39 | -6.84 | 6.39 | 3.82 | 260.05 | 0.0675 | -658.0 | -527.4 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -6.79 | 5.91 | 3.34 | 259.66 | 0.0590 | -880.0 | -723.1 | |
| 0.79 | 2.03 | 0.39 | 1.01 | -7.00 | 5.82 | 3.25 | 255.82 | 0.0583 | -1104.4 | -872.0 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -7.51 | 5.61 | 3.04 | 246.27 | 0.0577 | -836.0 | -634.2 | |
| 0.00 | 3.35 | 0.00 | 1.66 | -7.66 | 5.28 | 2.71 | 241.21 | 0.0537 | -1375.0 | -1020.5 | |
| 0.00 | 1.50 | 0.00 | 0.74 | -8.11 | 4.80 | 2.22 | 228.86 | 0.0513 | -707.0 | -556.5 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -7.72 | 3.95 | 1.37 | 221.63 | 0.0359 | -825.0 | -695.4 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -12.80 | 359.47 | -3.10 | 155.37 | 0.1272 | 839.0 | 599.6 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -12.64 | 358.89 | -3.69 | 150.86 | 0.1294 | 891.0 | 684.8 | |
| 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. | |