SDO HMI 2014-04-11 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.87 | 0.00 | 15.48 | -20.38 | 323.13 | 16.10 | 223.87 | 0.3811 | -312.5 | -132.9 | |
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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 | 1.59 | 0.00 | 0.88 | -16.66 | 332.46 | 25.42 | 244.47 | 0.4577 | 710.0 | 572.7 | |
| 0.00 | 1.15 | 0.00 | 0.64 | -17.56 | 332.42 | 25.38 | 242.62 | 0.4621 | 801.0 | 606.8 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -15.34 | 330.23 | 23.20 | 245.60 | 0.4188 | 545.0 | 456.5 | |
| 0.00 | 1.59 | 0.00 | 0.88 | -19.25 | 330.24 | 23.20 | 237.29 | 0.4438 | 821.0 | 600.1 | |
| 0.00 | 6.97 | 0.00 | 3.80 | -17.59 | 329.28 | 22.25 | 239.81 | 0.4193 | 826.0 | 649.4 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -22.34 | 320.41 | 13.37 | 216.82 | 0.3586 | -904.0 | -723.8 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -18.53 | 319.82 | 12.79 | 223.47 | 0.3063 | -846.0 | -693.4 | |
| 0.00 | 1.94 | 0.00 | 1.03 | -22.54 | 320.10 | 13.06 | 215.84 | 0.3580 | -822.0 | -683.2 | |
| 0.00 | 2.30 | 0.00 | 1.21 | -21.40 | 319.26 | 12.23 | 216.19 | 0.3354 | -1000.0 | -873.8 | |
| 0.00 | 2.12 | 0.00 | 1.11 | -20.41 | 318.69 | 11.66 | 216.84 | 0.3172 | -778.0 | -715.6 | |
| 0.00 | 2.65 | 0.00 | 1.40 | -24.24 | 316.57 | 9.53 | 205.53 | 0.3519 | -779.0 | -674.4 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -24.56 | 316.56 | 9.52 | 205.09 | 0.3564 | -651.0 | -619.3 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -22.64 | 316.42 | 9.38 | 207.48 | 0.3276 | -930.0 | -764.2 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -24.35 | 315.51 | 8.47 | 202.90 | 0.3464 | -866.0 | -716.2 | |
| 0.00 | 1.59 | 0.00 | 0.84 | -26.82 | 311.18 | 4.14 | 190.22 | 0.3648 | -815.0 | -664.0 | |
| 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. | |