SDO HMI 2014-11-11 21:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.84 | 0.00 | 6.75 | -9.06 | 338.14 | -14.29 | 130.72 | 0.3270 | -103.4 | -89.4 | |
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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 | 0.95 | 0.00 | 0.49 | -9.17 | 343.23 | -9.20 | 143.65 | 0.2674 | 949.0 | 794.8 | |
| 0.00 | 1.55 | 0.00 | 0.78 | -1.37 | 342.69 | -9.73 | 115.26 | 0.1877 | 923.0 | 716.4 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -9.30 | 342.10 | -10.33 | 140.73 | 0.2808 | 717.0 | 470.1 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -13.49 | 340.69 | -11.73 | 145.42 | 0.3499 | 652.0 | 511.6 | |
| 0.00 | 1.72 | 0.00 | 0.90 | -11.30 | 340.55 | -11.88 | 141.09 | 0.3228 | 782.0 | 623.5 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -9.70 | 336.71 | -15.72 | 129.74 | 0.3488 | -902.0 | -706.7 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -10.31 | 336.64 | -15.78 | 130.97 | 0.3560 | -981.0 | -745.4 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -8.96 | 335.27 | -17.16 | 125.66 | 0.3602 | -790.0 | -627.9 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -9.18 | 334.82 | -17.61 | 125.46 | 0.3682 | -750.0 | -638.2 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -10.69 | 334.06 | -18.36 | 127.56 | 0.3922 | -903.0 | -655.7 | |
| 0.00 | 1.55 | 0.00 | 0.83 | -8.29 | 334.17 | -18.26 | 122.45 | 0.3690 | -834.0 | -697.8 | |
| 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. | |