SDO HMI 2014-01-18 00:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.86 | 221.09 | 30.87 | 159.66 | -16.02 | 11.76 | 46.15 | 252.48 | 0.7293 | 744.6 | 303.2 | |
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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 |
| 23.30 | 134.77 | 17.00 | 98.56 | -16.47 | 12.36 | 46.75 | 251.99 | 0.7369 | 889.7 | 258.5 | |
| 0.00 | 1.53 | 0.00 | 1.10 | -14.69 | 11.75 | 46.14 | 254.29 | 0.7269 | 582.0 | 361.8 | |
| 18.28 | 77.29 | 12.97 | 54.78 | -14.98 | 10.95 | 45.34 | 253.75 | 0.7181 | 937.4 | 394.2 | |
| 1.28 | -3.00 | 0.90 | -3.00 | -14.60 | 10.72 | 45.11 | 254.23 | 0.7148 | 892.7 | 999999 | |
| 0.00 | 0.34 | 0.00 | 0.24 | -19.16 | 10.79 | 45.18 | 247.99 | 0.7251 | 562.0 | 571.8 | |
| 0.00 | 1.28 | 0.00 | 0.91 | -19.75 | 10.60 | 45.00 | 247.13 | 0.7246 | 488.0 | 410.3 | |
| 0.00 | 1.02 | 0.00 | 0.73 | -19.42 | 10.44 | 44.83 | 247.53 | 0.7219 | 623.0 | 568.6 | |
| 0.00 | 0.43 | 0.00 | 0.29 | -16.22 | 9.35 | 43.74 | 251.68 | 0.7017 | 477.0 | 407.4 | |
| 0.00 | 0.85 | 0.00 | 0.61 | -19.83 | 10.36 | 44.76 | 246.96 | 0.7221 | 585.0 | 501.2 | |
| 0.00 | 1.53 | 0.00 | 1.09 | -19.78 | 10.12 | 44.52 | 246.96 | 0.7193 | 737.0 | 635.3 | |
| 0.00 | 0.94 | 0.00 | 0.63 | -17.95 | 7.18 | 41.58 | 248.63 | 0.6804 | -447.0 | -338.2 | |
| 0.00 | 0.60 | 0.00 | 0.39 | -18.16 | 5.48 | 39.87 | 247.76 | 0.6605 | -521.0 | -469.4 | |
| 0.00 | 0.51 | 0.00 | 0.33 | -18.37 | 4.89 | 39.28 | 247.23 | 0.6540 | -739.0 | -583.7 | |
| 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. | |