SDO HMI 2014-03-06 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.13 | 164.44 | 32.34 | 147.30 | -10.13 | 359.71 | -57.11 | 97.39 | 0.8356 | 598.6 | 310.2 | |
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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 |
| 0.00 | 2.07 | 0.00 | 1.71 | -12.98 | 3.21 | -53.61 | 100.82 | 0.8009 | 574.0 | 469.1 | |
| 0.00 | 1.30 | 0.00 | 1.10 | -13.90 | 1.85 | -54.98 | 101.94 | 0.8147 | 425.0 | 407.3 | |
| 0.00 | 3.98 | 0.00 | 3.42 | -14.80 | 1.41 | -55.42 | 103.03 | 0.8193 | 107.0 | 91.3 | |
| 0.00 | 0.86 | 0.00 | 0.74 | -9.38 | 1.65 | -55.17 | 96.39 | 0.8172 | -292.0 | -269.3 | |
| 14.52 | 128.47 | 12.85 | 113.86 | -9.60 | 0.24 | -56.58 | 96.71 | 0.8309 | 818.8 | 355.3 | |
| 17.20 | -5.00 | 15.31 | -5.00 | -10.32 | 359.99 | -56.83 | 97.60 | 0.8330 | 826.3 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.17 | -9.67 | 359.55 | -57.27 | 96.84 | 0.8374 | 330.0 | 307.1 | |
| 0.00 | 0.95 | 0.00 | 0.87 | -9.87 | 358.87 | -57.95 | 97.11 | 0.8436 | 423.0 | 337.8 | |
| 0.52 | 1.56 | 0.49 | 1.47 | -10.93 | 357.79 | -59.03 | 98.41 | 0.8531 | 299.0 | 321.8 | |
| 0.00 | 3.03 | 0.00 | 2.88 | -10.21 | 357.49 | -59.34 | 97.57 | 0.8561 | 471.0 | 338.3 | |
| 3.89 | 14.18 | 3.69 | 13.42 | -9.14 | 357.68 | -59.15 | 96.31 | 0.8548 | 467.9 | 311.2 | |
| 0.00 | 1.64 | 0.00 | 1.57 | -9.93 | 357.45 | -59.37 | 97.25 | 0.8565 | 24.0 | -44.7 | |
| 0.00 | 2.59 | 0.00 | 2.54 | -10.24 | 356.45 | -60.38 | 97.66 | 0.8652 | -404.0 | -417.0 | |
| 0.00 | 0.61 | 0.00 | 0.59 | -7.74 | 356.96 | -59.86 | 94.73 | 0.8619 | 223.0 | 307.1 | |
| 0.00 | 0.86 | 0.00 | 0.86 | -11.08 | 355.85 | -60.98 | 98.66 | 0.8700 | 305.0 | 256.7 | |
| 0.00 | 1.04 | 0.00 | 1.10 | -14.44 | 353.74 | -63.08 | 102.54 | 0.8865 | -391.0 | -357.9 | |
| 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. | |