SDO HMI 2011-10-05 20:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.71 | 133.29 | 58.30 | 219.55 | -14.36 | 116.80 | -69.49 | 107.45 | 0.9514 | 129.6 | -127.5 | |
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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 |
| 10.54 | 56.19 | 14.74 | 84.45 | -13.99 | 119.60 | -66.69 | 107.66 | 0.9367 | 561.6 | -400.6 | |
| 0.00 | 1.23 | 0.00 | 1.77 | -14.13 | 118.96 | -67.33 | 107.66 | 0.9406 | 184.0 | 133.9 | |
| 0.00 | 3.34 | 0.00 | 4.94 | -14.53 | 118.46 | -67.83 | 107.96 | 0.9438 | -497.0 | -462.4 | |
| 7.46 | 18.97 | 10.85 | 28.09 | -13.87 | 118.71 | -67.58 | 107.33 | 0.9416 | 493.8 | 275.6 | |
| 0.00 | 4.30 | 0.00 | 6.26 | -13.41 | 118.57 | -67.72 | 106.83 | 0.9418 | 471.0 | 401.9 | |
| 0.00 | 3.78 | 0.00 | 5.65 | -14.19 | 118.10 | -68.20 | 107.53 | 0.9454 | -427.0 | -333.5 | |
| 4.65 | -4.00 | 6.99 | -4.00 | -13.75 | 118.03 | -68.26 | 107.07 | 0.9452 | 334.1 | 999999 | |
| 2.55 | -1.00 | 4.03 | -1.00 | -14.83 | 117.15 | -69.14 | 107.98 | 0.9511 | -723.9 | 999999 | |
| 0.00 | 0.97 | 0.00 | 1.49 | -13.52 | 117.32 | -68.97 | 106.67 | 0.9487 | 129.0 | 100.7 | |
| 1.32 | 1.76 | 2.08 | 2.77 | -13.66 | 116.88 | -69.41 | 106.72 | 0.9512 | -133.3 | -134.0 | |
| 0.97 | 3.51 | 1.72 | 6.19 | -15.52 | 115.13 | -71.16 | 108.28 | 0.9616 | 191.7 | -124.9 | |
| 2.81 | 38.63 | 5.28 | 76.78 | -15.04 | 114.03 | -72.26 | 107.57 | 0.9660 | -227.4 | 90.2 | |
| 0.00 | 0.61 | 0.00 | 1.16 | -14.09 | 113.78 | -72.51 | 106.55 | 0.9662 | -431.0 | -395.3 | |
| 5.27 | -12.00 | 10.33 | -12.00 | -14.69 | 113.28 | -73.01 | 107.06 | 0.9688 | -346.1 | 999999 | |
| 1.14 | -12.00 | 2.28 | -12.00 | -14.80 | 113.07 | -73.22 | 107.14 | 0.9698 | 253.2 | 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. | |