SDO HMI 2014-04-11 23:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.59 | 0.00 | 11.42 | -14.77 | 301.93 | 2.60 | 192.92 | 0.1942 | -207.8 | -165.9 | |
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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 | 0.71 | 0.00 | 0.36 | -15.01 | 311.49 | 12.16 | 231.66 | 0.2606 | 779.0 | 564.0 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -14.16 | 311.28 | 11.96 | 233.94 | 0.2496 | 718.0 | 579.0 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -15.04 | 311.24 | 11.91 | 230.98 | 0.2577 | 820.0 | 699.6 | |
| 0.00 | 4.41 | 0.00 | 2.24 | -12.14 | 310.65 | 11.33 | 239.94 | 0.2229 | 564.0 | 717.7 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -12.54 | 305.69 | 6.36 | 222.79 | 0.1599 | 782.0 | 575.3 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -15.51 | 299.08 | -0.24 | 178.60 | 0.1683 | -786.0 | -662.2 | |
| 0.00 | 3.44 | 0.00 | 1.72 | -13.54 | 298.41 | -0.92 | 173.34 | 0.1350 | -1109.0 | -809.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -14.33 | 298.37 | -0.95 | 173.75 | 0.1486 | -786.0 | -553.1 | |
| 0.00 | 1.59 | 0.00 | 0.80 | -17.01 | 297.54 | -1.79 | 171.23 | 0.1963 | -676.0 | -590.3 | |
| 0.00 | 1.76 | 0.00 | 0.89 | -16.82 | 297.32 | -2.00 | 170.01 | 0.1938 | -746.0 | -577.6 | |
| 0.00 | 2.21 | 0.00 | 1.12 | -17.09 | 296.79 | -2.54 | 167.72 | 0.2002 | -643.0 | -552.5 | |
| 0.00 | 2.65 | 0.00 | 1.34 | -17.36 | 295.65 | -3.68 | 162.92 | 0.2096 | -759.0 | -566.8 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -13.73 | 294.63 | -4.70 | 149.87 | 0.1592 | -859.0 | -676.3 | |
| 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. | |