SDO HMI 2014-04-06 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.67 | 17.59 | 0.98 | 10.89 | -16.04 | 329.45 | -35.87 | 108.50 | 0.5933 | 70.1 | 40.0 | |
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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 | 0.70 | 0.00 | 0.43 | -22.71 | 332.79 | -32.53 | 121.12 | 0.5817 | 39.0 | 135.0 | |
| 0.00 | 3.08 | 0.00 | 1.79 | -13.66 | 333.92 | -31.40 | 105.98 | 0.5287 | 505.0 | 453.8 | |
| 1.23 | 2.90 | 0.72 | 1.70 | -13.83 | 333.64 | -31.68 | 106.19 | 0.5331 | 791.5 | 552.7 | |
| 0.44 | 1.32 | 0.26 | 0.78 | -13.10 | 332.73 | -32.59 | 104.59 | 0.5442 | -762.2 | -656.5 | |
| 0.00 | 3.26 | 0.00 | 1.92 | -13.43 | 332.64 | -32.68 | 105.16 | 0.5462 | -984.0 | -753.7 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -18.43 | 330.20 | -35.12 | 112.88 | 0.5946 | 623.0 | 451.0 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -17.57 | 328.30 | -37.03 | 110.77 | 0.6162 | 654.0 | 518.4 | |
| 0.00 | 0.53 | 0.00 | 0.33 | -17.09 | 327.94 | -37.39 | 109.88 | 0.6194 | 576.0 | 470.3 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -18.94 | 326.90 | -38.42 | 112.41 | 0.6381 | 484.0 | 480.6 | |
| 0.00 | 1.67 | 0.00 | 1.07 | -17.37 | 326.63 | -38.69 | 109.91 | 0.6369 | 647.0 | 526.1 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -23.83 | 315.50 | -49.82 | 115.80 | 0.7785 | -291.0 | -378.7 | |
| 0.00 | 0.79 | 0.00 | 0.61 | -22.23 | 316.20 | -49.12 | 113.93 | 0.7680 | -537.0 | -442.6 | |
| 0.00 | 0.88 | 0.00 | 0.67 | -19.06 | 315.92 | -49.40 | 109.78 | 0.7649 | -416.0 | -399.3 | |
| 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. | |