SDO HMI 2014-05-10 07:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.10 | 272.68 | 27.64 | 175.50 | 14.77 | 249.30 | -35.69 | 62.11 | 0.6404 | -543.4 | -223.2 | |
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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 |
| 41.58 | 247.25 | 26.66 | 158.53 | 14.85 | 249.61 | -35.38 | 61.82 | 0.6372 | -1073.0 | -321.0 | |
| 1.52 | -1.00 | 0.98 | -1.00 | 14.44 | 249.38 | -35.61 | 62.54 | 0.6377 | -829.5 | 999999 | |
| 0.00 | 1.79 | 0.00 | 1.19 | 17.21 | 248.02 | -36.97 | 59.53 | 0.6688 | 683.0 | 585.9 | |
| 0.00 | 1.25 | 0.00 | 0.84 | 16.05 | 247.25 | -37.74 | 61.57 | 0.6712 | 553.0 | 410.1 | |
| 0.00 | 5.91 | 0.00 | 3.86 | 13.05 | 247.53 | -37.46 | 65.60 | 0.6529 | 758.0 | 609.7 | |
| 0.00 | 1.43 | 0.00 | 0.94 | 13.44 | 247.38 | -37.61 | 65.13 | 0.6565 | 656.0 | 524.9 | |
| 0.00 | 1.52 | 0.00 | 1.01 | 14.13 | 246.61 | -38.38 | 64.57 | 0.6689 | 781.0 | 640.8 | |
| 0.00 | 1.97 | 0.00 | 1.32 | 14.84 | 246.35 | -38.64 | 63.74 | 0.6754 | 617.0 | 482.1 | |
| 0.00 | 0.90 | 0.00 | 0.60 | 13.85 | 246.55 | -38.44 | 65.00 | 0.6683 | 505.0 | 431.4 | |
| 0.00 | 4.66 | 0.00 | 3.12 | 14.58 | 246.36 | -38.63 | 64.08 | 0.6740 | 706.0 | 580.5 | |
| 0.00 | 0.81 | 0.00 | 0.53 | 11.51 | 246.80 | -38.18 | 68.20 | 0.6547 | 642.0 | 484.6 | |
| 0.00 | 1.52 | 0.00 | 1.02 | 14.34 | 246.17 | -38.82 | 64.52 | 0.6751 | 714.0 | 583.1 | |
| 0.00 | 1.52 | 0.00 | 1.00 | 11.71 | 246.61 | -38.37 | 68.01 | 0.6579 | 782.0 | 655.0 | |
| 0.00 | 0.54 | 0.00 | 0.38 | 14.56 | 242.86 | -42.12 | 65.85 | 0.7138 | -170.0 | -32.8 | |
| 0.00 | 1.61 | 0.00 | 1.16 | 14.85 | 241.85 | -43.14 | 65.92 | 0.7262 | 110.0 | 248.2 | |
| 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. | |