SDO HMI 2014-05-10 01:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.22 | 265.51 | 30.95 | 178.32 | 14.75 | 249.52 | -38.76 | 63.87 | 0.6767 | -658.8 | -225.3 | |
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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 |
| 7.26 | 250.64 | 4.87 | 167.94 | 15.27 | 249.73 | -38.55 | 63.05 | 0.6768 | -864.9 | -276.3 | |
| 35.29 | -1.00 | 23.63 | -1.00 | 14.79 | 249.71 | -38.57 | 63.72 | 0.6747 | -1067.5 | 999999 | |
| 3.67 | -1.00 | 2.45 | -1.00 | 14.38 | 249.76 | -38.53 | 64.26 | 0.6721 | -1089.2 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.56 | 16.90 | 248.08 | -40.21 | 61.77 | 0.7034 | 661.0 | 480.8 | |
| 0.00 | 2.06 | 0.00 | 1.41 | 13.14 | 247.49 | -40.79 | 67.10 | 0.6930 | 650.0 | 571.3 | |
| 0.00 | 0.27 | 0.00 | 0.18 | 12.95 | 247.32 | -40.96 | 67.43 | 0.6942 | 542.0 | 473.0 | |
| 0.00 | 2.33 | 0.00 | 1.64 | 14.76 | 246.47 | -41.81 | 65.40 | 0.7114 | 670.0 | 586.7 | |
| 0.00 | 0.99 | 0.00 | 0.69 | 14.63 | 246.37 | -41.91 | 65.61 | 0.7120 | 711.0 | 612.5 | |
| 0.00 | 0.72 | 0.00 | 0.49 | 12.32 | 246.66 | -41.63 | 68.59 | 0.6994 | 573.0 | 483.1 | |
| 0.00 | 1.43 | 0.00 | 1.01 | 14.39 | 246.18 | -42.11 | 66.02 | 0.7131 | 497.0 | 463.1 | |
| 0.00 | 3.76 | 0.00 | 2.60 | 11.70 | 246.52 | -41.76 | 69.50 | 0.6986 | 667.0 | 548.1 | |
| 0.00 | 1.07 | 0.00 | 0.74 | 11.26 | 246.56 | -41.72 | 70.08 | 0.6965 | 665.0 | 486.8 | |
| 0.00 | 1.43 | 0.00 | 1.06 | 14.10 | 243.26 | -45.02 | 67.65 | 0.7441 | -508.0 | -374.0 | |
| 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. | |