SDO HMI 2011-01-05 04:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.90 | 413.32 | 42.57 | 255.07 | 31.32 | 188.34 | -11.59 | 16.75 | 0.5972 | -971.5 | -339.1 | |
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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 |
| 0.00 | 1.36 | 0.00 | 0.81 | 29.70 | 195.90 | -4.04 | 6.38 | 0.5527 | -729.0 | -543.1 | |
| 0.00 | 1.44 | 0.00 | 0.85 | 29.32 | 195.78 | -4.16 | 6.66 | 0.5473 | -666.0 | -541.9 | |
| 0.00 | 1.10 | 0.00 | 0.66 | 30.08 | 192.80 | -7.13 | 11.01 | 0.5648 | -683.0 | -612.0 | |
| 0.00 | 0.76 | 0.00 | 0.51 | 37.90 | 189.49 | -10.44 | 12.23 | 0.6778 | 609.0 | 525.7 | |
| 0.00 | 1.10 | 0.00 | 0.68 | 31.79 | 190.08 | -9.86 | 14.17 | 0.5969 | -516.0 | -323.8 | |
| 63.89 | 393.82 | 39.33 | 242.67 | 31.23 | 188.38 | -11.56 | 16.77 | 0.5958 | -1332.0 | -358.6 | |
| 0.00 | 1.10 | 0.00 | 0.72 | 34.99 | 187.42 | -12.51 | 15.95 | 0.6481 | 627.0 | 601.6 | |
| 0.00 | 3.48 | 0.00 | 2.27 | 35.19 | 187.17 | -12.77 | 16.15 | 0.6515 | 742.0 | 670.9 | |
| 0.51 | -6.00 | 0.31 | -6.00 | 30.92 | 187.75 | -12.18 | 17.81 | 0.5943 | -955.0 | 999999 | |
| 0.00 | 1.10 | 0.00 | 0.66 | 28.59 | 187.63 | -12.31 | 19.47 | 0.5640 | -684.0 | -523.0 | |
| 0.00 | 1.10 | 0.00 | 0.71 | 34.44 | 186.70 | -13.24 | 17.12 | 0.6439 | -504.0 | -437.2 | |
| 0.00 | 0.42 | 0.00 | 0.27 | 33.96 | 186.56 | -13.38 | 17.56 | 0.6384 | -567.0 | -468.4 | |
| 4.50 | 5.69 | 2.93 | 3.70 | 34.32 | 184.99 | -14.95 | 19.22 | 0.6495 | 779.9 | 678.4 | |
| 0.00 | 0.85 | 0.00 | 0.56 | 33.87 | 181.21 | -18.73 | 23.82 | 0.6625 | 710.0 | 552.0 | |
| 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. | |