SDO HMI 2011-06-07 05:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.08 | 63.21 | 22.84 | 59.67 | -21.19 | 36.70 | 55.70 | 244.74 | 0.8531 | 256.9 | 227.3 | |
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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 |
| 11.04 | 29.60 | 11.06 | 29.54 | -19.34 | 39.41 | 58.41 | 247.58 | 0.8714 | 628.8 | 430.5 | |
| 0.81 | 1.63 | 0.83 | 1.65 | -20.08 | 39.73 | 58.72 | 246.81 | 0.8752 | 165.9 | 155.0 | |
| 0.00 | 1.27 | 0.00 | 1.21 | -20.53 | 37.20 | 56.19 | 245.71 | 0.8557 | 640.0 | 545.0 | |
| 2.63 | 3.17 | 2.46 | 2.97 | -22.17 | 36.15 | 55.15 | 243.57 | 0.8508 | 371.2 | 255.3 | |
| 0.00 | 1.00 | 0.00 | 0.90 | -22.17 | 34.62 | 53.62 | 243.13 | 0.8379 | 560.0 | 476.1 | |
| 4.44 | 9.78 | 3.97 | 8.74 | -23.06 | 33.96 | 52.95 | 241.90 | 0.8346 | 569.2 | 424.1 | |
| 0.00 | 0.36 | 0.00 | 0.31 | -21.28 | 32.47 | 51.47 | 243.51 | 0.8166 | -400.0 | -512.5 | |
| 0.00 | 1.36 | 0.00 | 1.15 | -21.24 | 32.25 | 51.24 | 243.47 | 0.8145 | -550.0 | -476.3 | |
| 0.00 | 0.45 | 0.00 | 0.40 | -24.59 | 33.47 | 52.47 | 239.99 | 0.8349 | -475.0 | -446.2 | |
| 1.72 | 9.69 | 1.51 | 8.50 | -23.82 | 32.86 | 51.85 | 240.67 | 0.8274 | 116.4 | -164.9 | |
| 0.00 | 1.27 | 0.00 | 1.11 | -23.52 | 32.69 | 51.68 | 240.96 | 0.8251 | 166.0 | 65.8 | |
| 0.00 | 1.72 | 0.00 | 1.53 | -24.72 | 33.33 | 52.32 | 239.78 | 0.8341 | -626.0 | -569.9 | |
| 0.00 | 0.91 | 0.00 | 0.79 | -23.65 | 32.55 | 51.54 | 240.75 | 0.8242 | -432.0 | -367.4 | |
| 3.44 | -10.00 | 3.01 | -10.00 | -23.99 | 32.68 | 51.68 | 240.41 | 0.8264 | -297.0 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.87 | -24.25 | 32.29 | 51.29 | 239.97 | 0.8239 | -251.0 | -362.4 | |
| 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. | |