SDO HMI 2011-07-16 21:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.52 | 292.06 | 7.89 | 149.10 | 16.47 | 169.20 | -6.78 | 28.28 | 0.2388 | -448.0 | -469.4 | |
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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 |
| 2.27 | 277.00 | 1.15 | 141.24 | 16.23 | 169.61 | -6.37 | 27.53 | 0.2315 | -1560.3 | -522.7 | |
| 7.44 | -1.00 | 3.79 | -1.00 | 16.54 | 169.57 | -6.41 | 27.05 | 0.2365 | -1401.3 | 999999 | |
| 0.91 | -1.00 | 0.46 | -1.00 | 16.82 | 169.46 | -6.52 | 26.87 | 0.2415 | -970.3 | 999999 | |
| 4.90 | -1.00 | 2.49 | -1.00 | 16.01 | 169.36 | -6.62 | 28.90 | 0.2302 | -1473.0 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 17.18 | 168.03 | -7.94 | 30.87 | 0.2584 | -258.0 | -115.5 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 16.24 | 167.53 | -8.45 | 34.55 | 0.2499 | -870.0 | -636.2 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 21.03 | 165.60 | -10.38 | 30.44 | 0.3334 | 854.0 | 733.6 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.92 | 164.71 | -11.26 | 43.19 | 0.2757 | 526.0 | 463.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 20.06 | 164.31 | -11.67 | 35.10 | 0.3318 | 808.0 | 618.9 | |
| 0.00 | 2.18 | 0.00 | 1.14 | 19.60 | 163.32 | -12.66 | 38.15 | 0.3357 | 822.0 | 652.3 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 23.65 | 161.13 | -14.84 | 35.34 | 0.4074 | 730.0 | 619.9 | |
| 0.00 | 3.45 | 0.00 | 1.81 | 17.93 | 161.47 | -14.51 | 45.38 | 0.3363 | 736.0 | 663.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 13.38 | 160.99 | -14.99 | 57.94 | 0.2982 | 828.0 | 677.9 | |
| 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. | |