SDO HMI 2014-04-01 08:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.38 | 0.00 | 12.29 | -16.92 | 123.79 | 44.24 | 251.47 | 0.6980 | 23.1 | 39.6 | |
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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 | 0.61 | 0.00 | 0.50 | -13.03 | 132.43 | 52.88 | 258.56 | 0.7948 | 413.0 | 385.4 | |
| 0.00 | 0.53 | 0.00 | 0.44 | -16.51 | 133.35 | 53.80 | 254.27 | 0.8060 | 510.0 | 474.5 | |
| 0.00 | 2.37 | 0.00 | 1.95 | -15.88 | 132.78 | 53.23 | 255.00 | 0.7999 | 530.0 | 460.3 | |
| 0.00 | 1.67 | 0.00 | 1.41 | -18.55 | 133.80 | 54.26 | 251.80 | 0.8122 | 194.0 | 181.5 | |
| 0.00 | 0.70 | 0.00 | 0.59 | -17.77 | 133.40 | 53.85 | 252.71 | 0.8076 | 524.0 | 409.2 | |
| 0.00 | 0.97 | 0.00 | 0.79 | -15.90 | 132.53 | 52.98 | 254.95 | 0.7974 | 615.0 | 575.7 | |
| 0.00 | 0.97 | 0.00 | 0.74 | -9.63 | 130.03 | 50.48 | 262.89 | 0.7687 | 574.0 | 495.9 | |
| 0.00 | 1.23 | 0.00 | 0.85 | -11.45 | 124.44 | 44.89 | 260.30 | 0.7041 | 457.0 | 469.4 | |
| 0.00 | 0.35 | 0.00 | 0.22 | -18.88 | 114.86 | 35.31 | 246.86 | 0.5969 | -685.0 | -556.2 | |
| 0.00 | 3.51 | 0.00 | 2.18 | -20.52 | 114.84 | 35.29 | 244.22 | 0.6032 | -678.0 | -461.7 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -20.47 | 114.63 | 35.09 | 244.20 | 0.6004 | -648.0 | -525.4 | |
| 0.00 | 1.58 | 0.00 | 0.89 | -10.56 | 108.18 | 28.63 | 259.90 | 0.4804 | -736.0 | -525.3 | |
| 0.00 | 1.84 | 0.00 | 1.08 | -23.61 | 108.43 | 28.88 | 235.28 | 0.5406 | -770.0 | -550.0 | |
| 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. | |