SDO HMI 2014-04-03 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.40 | 355.90 | 40.14 | 241.09 | 12.42 | 13.76 | -38.86 | 64.01 | 0.6839 | -702.7 | -292.0 | |
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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 |
| 54.13 | 336.49 | 36.51 | 227.37 | 12.46 | 14.06 | -38.56 | 63.78 | 0.6807 | -1187.6 | -345.9 | |
| 5.27 | -1.00 | 3.63 | -1.00 | 12.65 | 12.83 | -39.78 | 64.24 | 0.6956 | -569.3 | 999999 | |
| 0.00 | 1.93 | 0.00 | 1.33 | 11.66 | 12.53 | -40.09 | 65.72 | 0.6942 | -454.0 | -294.0 | |
| 0.00 | 1.14 | 0.00 | 0.79 | 11.15 | 11.40 | -41.21 | 66.98 | 0.7047 | 728.0 | 609.4 | |
| 0.00 | 0.97 | 0.00 | 0.67 | 10.52 | 11.47 | -41.15 | 67.79 | 0.7011 | 371.0 | 386.6 | |
| 0.00 | 1.23 | 0.00 | 0.87 | 12.24 | 11.12 | -41.49 | 65.69 | 0.7128 | 561.0 | 482.2 | |
| 0.00 | 2.11 | 0.00 | 1.47 | 10.72 | 11.35 | -41.26 | 67.58 | 0.7033 | 555.0 | 467.7 | |
| 0.00 | 1.23 | 0.00 | 0.86 | 11.99 | 11.09 | -41.53 | 66.03 | 0.7120 | 755.0 | 629.9 | |
| 0.00 | 0.35 | 0.00 | 0.25 | 11.78 | 11.05 | -41.57 | 66.34 | 0.7115 | 517.0 | 594.0 | |
| 0.00 | 1.32 | 0.00 | 0.92 | 10.98 | 11.15 | -41.47 | 67.33 | 0.7068 | 703.0 | 591.4 | |
| 0.00 | 1.14 | 0.00 | 0.80 | 11.66 | 10.86 | -41.75 | 66.58 | 0.7131 | 717.0 | 523.5 | |
| 0.00 | 2.28 | 0.00 | 1.60 | 11.04 | 10.89 | -41.72 | 67.39 | 0.7100 | 608.0 | 495.8 | |
| 0.00 | 0.88 | 0.00 | 0.62 | 11.66 | 10.49 | -42.13 | 66.77 | 0.7172 | 567.0 | 512.6 | |
| 0.00 | 0.44 | 0.00 | 0.31 | 11.56 | 10.18 | -42.44 | 67.05 | 0.7203 | 439.0 | 324.2 | |
| 0.00 | 0.70 | 0.00 | 0.48 | 3.94 | 10.95 | -41.67 | 77.13 | 0.6827 | 621.0 | 465.8 | |
| 0.00 | 3.69 | 0.00 | 2.75 | 12.87 | 8.04 | -44.58 | 66.41 | 0.7490 | 690.0 | 558.0 | |
| 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. | |