SDO HMI 2014-04-11 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.77 | 0.00 | 10.48 | -21.49 | 322.05 | 11.18 | 211.86 | 0.3515 | -131.6 | -167.9 | |
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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 | 1.32 | 0.00 | 0.72 | -16.51 | 332.65 | 21.77 | 241.81 | 0.4052 | 620.0 | 441.4 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -16.63 | 332.49 | 21.62 | 241.37 | 0.4039 | 658.0 | 552.5 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -16.79 | 332.41 | 21.53 | 240.94 | 0.4038 | 710.0 | 687.4 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -20.04 | 332.08 | 21.21 | 233.62 | 0.4239 | 573.0 | 518.5 | |
| 0.00 | 1.50 | 0.00 | 0.82 | -19.89 | 331.99 | 21.12 | 233.83 | 0.4215 | 709.0 | 636.1 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -19.68 | 325.16 | 14.28 | 223.98 | 0.3360 | 873.0 | 677.5 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -22.46 | 320.08 | 9.21 | 207.36 | 0.3231 | -754.0 | -634.7 | |
| 0.00 | 2.47 | 0.00 | 1.28 | -21.19 | 319.06 | 8.18 | 206.67 | 0.2970 | -812.0 | -663.0 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -20.51 | 318.76 | 7.89 | 206.96 | 0.2847 | -777.0 | -680.8 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -23.85 | 316.80 | 5.92 | 197.03 | 0.3237 | -761.0 | -593.2 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -24.45 | 316.56 | 5.68 | 195.82 | 0.3321 | -637.0 | -525.2 | |
| 0.00 | 2.03 | 0.00 | 1.06 | -23.67 | 316.29 | 5.42 | 195.84 | 0.3185 | -975.0 | -693.3 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -23.62 | 312.15 | 1.28 | 183.85 | 0.3059 | -575.0 | -593.2 | |
| 0.00 | 2.56 | 0.00 | 1.36 | -26.77 | 311.38 | 0.50 | 181.26 | 0.3574 | -694.0 | -612.0 | |
| 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. | |