SDO HMI 2011-10-05 23:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.49 | 157.38 | 52.12 | 238.92 | -14.58 | 116.41 | -68.22 | 107.95 | 0.9452 | 27.1 | -78.3 | |
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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 |
| 7.47 | 24.94 | 9.72 | 32.50 | -14.15 | 119.74 | -64.89 | 108.25 | 0.9262 | 665.8 | 357.9 | |
| 1.05 | 1.84 | 1.41 | 2.46 | -14.29 | 119.07 | -65.57 | 108.23 | 0.9305 | 163.0 | 162.9 | |
| 2.37 | 10.19 | 3.23 | 13.89 | -14.64 | 118.71 | -65.92 | 108.51 | 0.9331 | -442.1 | -438.1 | |
| 7.82 | 16.07 | 10.45 | 21.73 | -13.94 | 119.04 | -65.60 | 107.86 | 0.9302 | 574.0 | 359.1 | |
| 0.00 | 7.20 | 0.00 | 9.60 | -13.51 | 118.97 | -65.67 | 107.39 | 0.9300 | 447.0 | 394.3 | |
| 0.00 | 1.32 | 0.00 | 1.81 | -14.17 | 118.37 | -66.27 | 107.94 | 0.9345 | -303.0 | -315.9 | |
| 2.81 | 35.31 | 4.14 | 51.75 | -14.95 | 117.01 | -67.63 | 108.44 | 0.9433 | -661.4 | -520.0 | |
| 2.55 | -7.00 | 3.80 | -7.00 | -14.83 | 116.67 | -67.96 | 108.24 | 0.9449 | -698.3 | 999999 | |
| 1.41 | 6.32 | 2.02 | 9.01 | -13.57 | 117.21 | -67.43 | 107.05 | 0.9404 | 110.1 | 216.1 | |
| 1.76 | 3.95 | 2.83 | 6.38 | -15.49 | 115.25 | -69.38 | 108.61 | 0.9531 | -251.1 | -78.5 | |
| 0.00 | 1.41 | 0.00 | 2.33 | -14.96 | 114.56 | -70.08 | 107.92 | 0.9559 | -468.0 | -417.4 | |
| 0.61 | 48.83 | 1.05 | 87.46 | -15.11 | 114.07 | -70.57 | 107.97 | 0.9584 | 59.3 | -41.5 | |
| 2.28 | -12.00 | 3.94 | -12.00 | -15.12 | 113.96 | -70.67 | 107.97 | 0.9589 | -264.7 | 999999 | |
| 4.22 | -12.00 | 7.47 | -12.00 | -14.74 | 113.39 | -71.24 | 107.46 | 0.9612 | -412.9 | 999999 | |
| 1.14 | -12.00 | 2.06 | -12.00 | -14.78 | 113.07 | -71.57 | 107.43 | 0.9627 | 238.5 | 999999 | |
| 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. | |