SDO HMI 2011-10-11 23:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 109.32 | 632.09 | 83.82 | 482.94 | 26.93 | 58.14 | -47.33 | 59.49 | 0.7628 | -926.7 | -293.5 | |
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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 | 1.05 | 0.00 | 0.77 | 27.29 | 60.61 | -44.87 | 58.20 | 0.7399 | 388.0 | 320.3 | |
| 0.88 | 611.53 | 0.65 | 465.02 | 27.75 | 59.74 | -45.74 | 57.93 | 0.7502 | -235.1 | -313.3 | |
| 1.40 | -2.00 | 1.03 | -2.00 | 26.71 | 60.19 | -45.28 | 59.11 | 0.7420 | -753.3 | 999999 | |
| 98.11 | -2.00 | 74.50 | -2.00 | 27.00 | 58.43 | -47.04 | 59.34 | 0.7604 | -1161.6 | 999999 | |
| 3.94 | -2.00 | 3.06 | -2.00 | 27.50 | 57.30 | -48.18 | 59.07 | 0.7729 | -322.1 | 999999 | |
| 1.40 | -2.00 | 1.07 | -2.00 | 26.52 | 57.70 | -47.77 | 60.18 | 0.7660 | -533.9 | 999999 | |
| 0.00 | 5.25 | 0.00 | 3.97 | 24.84 | 58.05 | -47.42 | 62.22 | 0.7577 | 424.0 | 373.9 | |
| 0.00 | 0.61 | 0.00 | 0.48 | 26.80 | 56.68 | -48.79 | 60.13 | 0.7766 | -11.0 | -95.6 | |
| 0.00 | 0.35 | 0.00 | 0.29 | 28.78 | 55.03 | -50.44 | 58.19 | 0.7974 | -497.0 | -449.5 | |
| 0.00 | 1.31 | 0.00 | 1.01 | 24.83 | 57.16 | -48.31 | 62.48 | 0.7665 | 623.0 | 467.7 | |
| 0.00 | 0.96 | 0.00 | 0.76 | 26.88 | 55.92 | -49.56 | 60.27 | 0.7840 | -220.0 | -214.8 | |
| 0.00 | 1.58 | 0.00 | 1.26 | 26.89 | 55.70 | -49.77 | 60.31 | 0.7861 | -533.0 | -360.4 | |
| 0.00 | 1.14 | 0.00 | 1.16 | 26.06 | 45.05 | -60.43 | 63.50 | 0.8750 | 487.0 | 372.7 | |
| 3.59 | 6.30 | 3.51 | 6.15 | 23.56 | 46.07 | -59.41 | 66.22 | 0.8643 | 517.1 | 284.4 | |
| 0.00 | 2.01 | 0.00 | 2.07 | 23.29 | 44.14 | -61.33 | 66.76 | 0.8790 | 531.0 | 393.8 | |
| 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. | |