SDO HMI 2011-06-02 10:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.37 | 155.11 | 17.10 | 90.39 | -20.65 | 19.11 | -25.33 | 130.76 | 0.5302 | 601.4 | 432.9 | |
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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 | 0.81 | 0.00 | 0.45 | -18.56 | 23.39 | -21.04 | 132.34 | 0.4623 | -577.0 | -446.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -17.92 | 22.93 | -21.51 | 130.65 | 0.4617 | -727.0 | -596.1 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -19.27 | 22.57 | -21.86 | 132.47 | 0.4785 | -808.0 | -630.7 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -19.46 | 22.30 | -22.13 | 132.45 | 0.4834 | -857.0 | -604.3 | |
| 1.08 | 136.12 | 0.63 | 79.11 | -20.81 | 19.68 | -24.75 | 131.59 | 0.5253 | 810.5 | 497.1 | |
| 25.31 | -5.00 | 14.72 | -5.00 | -20.52 | 19.38 | -25.06 | 130.81 | 0.5262 | 1171.3 | 999999 | |
| 2.98 | -5.00 | 1.75 | -5.00 | -20.84 | 18.71 | -25.73 | 130.61 | 0.5365 | 831.2 | 999999 | |
| 0.00 | 6.33 | 0.00 | 3.73 | -21.29 | 18.29 | -26.14 | 130.88 | 0.5450 | 749.0 | 636.2 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -20.87 | 18.23 | -26.21 | 130.18 | 0.5421 | 519.0 | 339.0 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -20.64 | 18.02 | -26.42 | 129.62 | 0.5426 | 608.0 | 424.4 | |
| 0.00 | 2.08 | 0.00 | 1.24 | -21.78 | 17.36 | -27.08 | 130.67 | 0.5595 | 591.0 | 439.8 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -21.19 | 17.47 | -26.96 | 129.92 | 0.5533 | 732.0 | 610.7 | |
| 0.00 | 1.27 | 0.00 | 0.80 | -23.37 | 12.62 | -31.81 | 128.82 | 0.6233 | -732.0 | -664.6 | |
| 0.00 | 1.63 | 0.00 | 1.04 | -24.03 | 12.09 | -32.35 | 129.30 | 0.6338 | -690.0 | -511.7 | |
| 0.00 | 1.18 | 0.00 | 0.74 | -22.12 | 11.98 | -32.46 | 126.60 | 0.6215 | -514.0 | -509.5 | |
| 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. | |