SDO HMI 2014-11-10 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.51 | 0.00 | 11.48 | -23.71 | 8.77 | -5.62 | 168.99 | 0.4666 | 657.0 | 540.4 | |
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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 | 1.21 | 0.00 | 0.66 | -20.70 | 10.26 | -4.13 | 170.63 | 0.4157 | 957.0 | 681.9 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -20.47 | 9.95 | -4.44 | 169.83 | 0.4130 | 813.0 | 631.7 | |
| 0.00 | 2.07 | 0.00 | 1.14 | -22.57 | 9.75 | -4.64 | 170.32 | 0.4462 | 825.0 | 692.6 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -23.60 | 9.52 | -4.87 | 170.27 | 0.4626 | 716.0 | 555.7 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -22.70 | 9.49 | -4.90 | 169.84 | 0.4490 | 846.0 | 712.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -23.24 | 9.47 | -4.92 | 170.02 | 0.4572 | 690.0 | 506.1 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -20.47 | 9.47 | -4.92 | 168.77 | 0.4145 | 609.0 | 469.8 | |
| 0.00 | 2.50 | 0.00 | 1.41 | -24.78 | 9.08 | -5.31 | 169.90 | 0.4817 | 733.0 | 585.2 | |
| 0.00 | 2.41 | 0.00 | 1.35 | -24.00 | 9.08 | -5.31 | 169.59 | 0.4700 | 823.0 | 765.5 | |
| 0.00 | 2.93 | 0.00 | 1.65 | -24.47 | 8.99 | -5.40 | 169.62 | 0.4773 | 831.0 | 686.5 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -24.27 | 8.77 | -5.62 | 169.12 | 0.4749 | 883.0 | 752.2 | |
| 0.00 | 1.98 | 0.00 | 1.13 | -25.35 | 8.62 | -5.77 | 169.31 | 0.4916 | 623.0 | 526.6 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -24.44 | 8.57 | -5.82 | 168.81 | 0.4781 | 692.0 | 482.2 | |
| 0.00 | 1.47 | 0.00 | 0.85 | -26.32 | 2.77 | -11.62 | 159.96 | 0.5290 | -843.0 | -682.8 | |
| 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. | |