SDO HMI 2011-06-07 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.30 | 39.82 | 15.88 | 42.80 | -20.94 | 36.96 | 60.34 | 246.13 | 0.8888 | 392.1 | 253.3 | |
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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 | 0.72 | 0.00 | 0.85 | -19.21 | 40.07 | 63.46 | 248.69 | 0.9086 | 327.0 | 345.1 | |
| 10.77 | 18.19 | 12.36 | 20.83 | -19.24 | 39.38 | 62.76 | 248.54 | 0.9038 | 570.8 | 421.4 | |
| 0.00 | 1.63 | 0.00 | 1.79 | -20.56 | 37.85 | 61.24 | 246.80 | 0.8948 | 326.0 | 221.6 | |
| 0.00 | 0.90 | 0.00 | 0.98 | -20.72 | 37.22 | 60.61 | 246.49 | 0.8905 | 233.0 | 303.1 | |
| 0.00 | 1.27 | 0.00 | 1.33 | -22.23 | 36.01 | 59.40 | 244.56 | 0.8842 | 511.0 | 354.6 | |
| 0.00 | 1.09 | 0.00 | 1.10 | -21.77 | 34.81 | 58.19 | 244.80 | 0.8742 | 664.0 | 557.1 | |
| 0.00 | 1.72 | 0.00 | 1.74 | -21.90 | 34.83 | 58.22 | 244.65 | 0.8747 | 697.0 | 621.0 | |
| 0.00 | 1.90 | 0.00 | 1.93 | -22.39 | 34.78 | 58.17 | 244.09 | 0.8752 | 464.0 | 429.1 | |
| 3.53 | 5.97 | 3.52 | 5.96 | -23.05 | 33.91 | 57.30 | 243.14 | 0.8699 | 462.7 | 172.3 | |
| 0.00 | 0.90 | 0.00 | 0.87 | -21.43 | 32.89 | 56.28 | 244.69 | 0.8585 | -422.0 | -308.9 | |
| 0.00 | 1.09 | 0.00 | 1.06 | -23.58 | 32.86 | 56.25 | 242.26 | 0.8630 | 261.0 | 208.8 | |
| 0.00 | 1.27 | 0.00 | 1.27 | -24.85 | 33.62 | 57.00 | 241.05 | 0.8716 | -422.0 | -329.0 | |
| 0.00 | 1.99 | 0.00 | 1.94 | -23.95 | 32.74 | 56.13 | 241.82 | 0.8629 | 70.0 | -42.3 | |
| 0.00 | 1.18 | 0.00 | 1.15 | -24.48 | 32.62 | 56.01 | 241.19 | 0.8632 | -462.0 | -529.7 | |
| 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. | |