SDO HMI 2011-06-01 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.38 | 53.03 | 6.57 | 28.17 | 17.10 | 41.58 | -11.11 | 30.82 | 0.3601 | -435.4 | -325.1 | |
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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 |
| 7.14 | 17.25 | 3.77 | 9.13 | 18.01 | 44.12 | -8.57 | 23.91 | 0.3511 | -1122.3 | -331.0 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 17.66 | 43.95 | -8.75 | 24.79 | 0.3471 | -1147.0 | -950.8 | |
| 2.62 | 8.22 | 1.38 | 4.33 | 17.21 | 43.65 | -9.05 | 26.12 | 0.3427 | -1074.6 | -876.7 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 16.90 | 43.15 | -9.55 | 27.80 | 0.3418 | -988.0 | -759.9 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 16.14 | 41.64 | -11.05 | 32.57 | 0.3436 | -1091.0 | -895.9 | |
| 0.00 | 4.34 | 0.00 | 2.29 | 15.92 | 41.40 | -11.30 | 33.50 | 0.3428 | -788.0 | -685.8 | |
| 0.00 | 2.80 | 0.00 | 1.48 | 15.66 | 40.54 | -12.15 | 35.87 | 0.3475 | -800.0 | -566.8 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 16.23 | 40.44 | -12.25 | 35.10 | 0.3559 | -749.0 | -615.7 | |
| 0.00 | 1.99 | 0.00 | 1.05 | 15.44 | 40.17 | -12.53 | 37.08 | 0.3483 | -918.0 | -699.1 | |
| 1.63 | 3.34 | 0.88 | 1.80 | 17.39 | 37.68 | -15.02 | 38.67 | 0.3975 | 1015.6 | 831.6 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 19.26 | 36.44 | -16.26 | 37.87 | 0.4323 | 742.0 | 629.9 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 16.28 | 36.65 | -16.05 | 42.41 | 0.3951 | 879.0 | 674.4 | |
| 0.00 | 3.07 | 0.00 | 1.65 | 15.77 | 36.62 | -16.07 | 43.37 | 0.3896 | 712.0 | 542.5 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 16.60 | 36.19 | -16.50 | 42.63 | 0.4037 | 801.0 | 641.7 | |
| 0.99 | 1.99 | 0.54 | 1.09 | 17.18 | 34.94 | -17.75 | 43.66 | 0.4238 | 957.8 | 844.1 | |
| 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. | |