SDO HMI 2014-12-05 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.43 | 0.00 | 10.41 | 13.49 | 16.78 | -25.36 | 61.40 | 0.4772 | -629.3 | -480.5 | |
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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 |
| 0.00 | 0.85 | 0.00 | 0.47 | 14.68 | 21.73 | -20.41 | 53.66 | 0.4206 | -718.0 | -663.3 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 16.52 | 20.69 | -21.46 | 51.49 | 0.4501 | -544.0 | -505.5 | |
| 0.00 | 4.78 | 0.00 | 2.66 | 13.74 | 18.54 | -23.60 | 59.16 | 0.4549 | -940.0 | -624.0 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 13.22 | 17.80 | -24.35 | 60.89 | 0.4613 | -808.0 | -652.4 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 13.49 | 17.47 | -24.68 | 60.67 | 0.4676 | -712.0 | -583.0 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 9.70 | 17.52 | -24.62 | 68.33 | 0.4438 | -850.0 | -700.7 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 8.92 | 17.51 | -24.63 | 70.01 | 0.4400 | -765.0 | -606.4 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 9.97 | 17.37 | -24.78 | 67.88 | 0.4474 | -629.0 | -488.8 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 9.10 | 17.37 | -24.77 | 69.73 | 0.4430 | -798.0 | -665.2 | |
| 0.00 | 1.88 | 0.00 | 1.07 | 13.25 | 15.50 | -26.64 | 62.83 | 0.4926 | -663.0 | -534.8 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 16.95 | 13.07 | -29.07 | 58.35 | 0.5482 | -603.0 | -460.7 | |
| 0.00 | 1.88 | 0.00 | 1.17 | 19.21 | 9.21 | -32.93 | 57.72 | 0.6095 | 478.0 | 403.0 | |
| 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. | |