SDO HMI 2014-04-11 03:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.89 | 127.88 | 39.01 | 181.81 | 4.33 | 241.44 | -68.88 | 83.11 | 0.9376 | -89.2 | -18.3 | |
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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 |
| 3.18 | 63.19 | 4.03 | 80.92 | 4.93 | 244.07 | -66.25 | 82.08 | 0.9224 | -892.9 | -321.5 | |
| 5.12 | -1.00 | 6.45 | -1.00 | 4.40 | 244.17 | -66.15 | 82.63 | 0.9212 | -682.1 | 999999 | |
| 2.21 | -1.00 | 2.81 | -1.00 | 4.73 | 243.96 | -66.36 | 82.31 | 0.9229 | -833.1 | 999999 | |
| 2.21 | -1.00 | 2.85 | -1.00 | 5.01 | 243.60 | -66.73 | 82.07 | 0.9256 | -385.0 | 999999 | |
| 0.26 | -1.00 | 0.34 | -1.00 | 4.80 | 243.48 | -66.84 | 82.31 | 0.9261 | -299.0 | 999999 | |
| 2.38 | -1.00 | 3.09 | -1.00 | 4.47 | 243.47 | -66.85 | 82.67 | 0.9259 | -368.0 | 999999 | |
| 1.41 | 6.44 | 1.84 | 8.41 | 4.17 | 243.37 | -66.96 | 83.00 | 0.9263 | -289.4 | -85.5 | |
| 0.00 | 1.24 | 0.00 | 1.81 | 5.54 | 240.94 | -69.39 | 81.92 | 0.9424 | -168.0 | -75.0 | |
| 0.00 | 0.97 | 0.00 | 1.42 | 4.46 | 240.76 | -69.57 | 83.09 | 0.9426 | 402.0 | 401.5 | |
| 0.00 | 2.91 | 0.00 | 4.35 | 3.18 | 240.19 | -70.13 | 84.52 | 0.9448 | 311.0 | 331.9 | |
| 2.12 | 47.30 | 3.25 | 74.54 | 3.96 | 239.69 | -70.63 | 83.77 | 0.9482 | 736.2 | 239.9 | |
| 8.47 | -11.00 | 13.41 | -11.00 | 3.89 | 239.14 | -71.18 | 83.91 | 0.9511 | 465.0 | 999999 | |
| 0.00 | 3.62 | 0.00 | 6.44 | 5.24 | 237.21 | -73.12 | 82.78 | 0.9618 | 234.0 | 225.2 | |
| 0.53 | 2.21 | 0.94 | 3.92 | 4.82 | 237.12 | -73.21 | 83.23 | 0.9619 | 185.7 | 149.2 | |
| 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. | |