SDO HMI 2014-01-18 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.28 | 214.48 | 28.56 | 156.43 | -16.06 | 11.75 | 46.69 | 252.53 | 0.7355 | 808.1 | 328.3 | |
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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 |
| 0.68 | 131.29 | 0.50 | 96.91 | -16.13 | 12.52 | 47.47 | 252.59 | 0.7442 | 562.0 | 299.3 | |
| 17.26 | -1.00 | 12.73 | -1.00 | -16.50 | 12.37 | 47.31 | 252.06 | 0.7432 | 887.2 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.74 | -14.64 | 11.72 | 46.66 | 254.46 | 0.7328 | 362.0 | 339.2 | |
| 3.06 | -1.00 | 2.24 | -1.00 | -16.46 | 12.04 | 46.98 | 252.05 | 0.7394 | 1052.9 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.42 | -13.90 | 10.86 | 45.81 | 255.32 | 0.7219 | 431.0 | 455.1 | |
| 18.28 | 73.39 | 13.09 | 52.54 | -14.96 | 10.92 | 45.87 | 253.88 | 0.7241 | 974.0 | 387.6 | |
| 0.00 | 2.04 | 0.00 | 1.48 | -19.13 | 10.86 | 45.80 | 248.20 | 0.7319 | 478.0 | 399.6 | |
| 0.00 | 0.94 | 0.00 | 0.68 | -19.79 | 10.60 | 45.55 | 247.24 | 0.7308 | 441.0 | 407.5 | |
| 0.00 | 1.11 | 0.00 | 0.80 | -19.49 | 10.45 | 45.40 | 247.60 | 0.7283 | 601.0 | 516.2 | |
| 0.00 | 1.11 | 0.00 | 0.80 | -19.90 | 10.37 | 45.32 | 247.04 | 0.7285 | 597.0 | 520.4 | |
| 0.00 | 1.70 | 0.00 | 1.22 | -19.82 | 10.12 | 45.07 | 247.07 | 0.7255 | 630.0 | 572.0 | |
| 0.00 | 1.28 | 0.00 | 0.84 | -18.17 | 4.89 | 39.84 | 247.74 | 0.6600 | -680.0 | -618.2 | |
| 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. | |