SDO HMI 2014-03-10 22:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.19 | 20.97 | 8.19 | 23.10 | -8.62 | 297.97 | -63.94 | 96.06 | 0.8941 | -106.4 | -37.7 | |
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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 | 0.52 | -12.66 | 306.65 | -55.26 | 100.41 | 0.8174 | 471.0 | 372.6 | |
| 0.00 | 0.95 | 0.00 | 0.82 | -11.19 | 306.19 | -55.73 | 98.62 | 0.8221 | 448.0 | 362.0 | |
| 0.00 | 1.21 | 0.00 | 1.18 | -10.86 | 301.74 | -60.18 | 98.37 | 0.8632 | 324.0 | 238.5 | |
| 1.73 | 4.07 | 1.79 | 4.19 | -6.70 | 300.09 | -61.82 | 93.71 | 0.8793 | 487.2 | 269.7 | |
| 0.00 | 0.87 | 0.00 | 0.92 | -6.84 | 299.15 | -62.77 | 93.94 | 0.8868 | 385.0 | 366.1 | |
| 0.00 | 0.43 | 0.00 | 0.47 | -6.53 | 298.55 | -63.36 | 93.65 | 0.8918 | 187.0 | 166.6 | |
| 0.43 | 1.30 | 0.48 | 1.44 | -6.56 | 298.00 | -63.92 | 93.73 | 0.8960 | 263.6 | 243.7 | |
| 0.00 | 0.61 | 0.00 | 0.68 | -8.89 | 297.33 | -64.58 | 96.39 | 0.8998 | -285.0 | -265.1 | |
| 0.00 | 0.69 | 0.00 | 0.78 | -8.09 | 297.45 | -64.47 | 95.49 | 0.8993 | -463.0 | -407.5 | |
| 5.03 | 7.28 | 5.92 | 8.58 | -9.37 | 296.00 | -65.92 | 97.01 | 0.9094 | -619.4 | -427.3 | |
| 0.00 | 1.30 | 0.00 | 1.55 | -9.07 | 295.73 | -66.18 | 96.70 | 0.9114 | -319.0 | -307.7 | |
| 0.00 | 0.52 | 0.00 | 0.62 | -9.34 | 295.48 | -66.44 | 97.02 | 0.9130 | -167.0 | -146.2 | |
| 0.00 | 1.13 | 0.00 | 1.35 | -8.22 | 295.65 | -66.26 | 95.77 | 0.9124 | -218.0 | -319.8 | |
| 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. | |