SDO HMI 2014-11-12 09:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.51 | 60.28 | 8.49 | 33.07 | -8.73 | 323.30 | -22.54 | 118.06 | 0.4313 | 920.3 | 613.9 | |
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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 | 1.46 | 0.00 | 0.79 | -7.66 | 324.61 | -21.23 | 117.17 | 0.4051 | 609.0 | 463.5 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -11.46 | 323.44 | -22.40 | 123.63 | 0.4504 | 898.0 | 686.4 | |
| 6.55 | 45.90 | 3.58 | 25.15 | -8.74 | 323.55 | -22.29 | 118.35 | 0.4278 | 1250.6 | 614.9 | |
| 7.84 | -3.00 | 4.30 | -3.00 | -8.75 | 323.35 | -22.49 | 118.15 | 0.4306 | 1038.1 | 999999 | |
| 0.00 | 2.58 | 0.00 | 1.42 | -8.36 | 323.22 | -22.63 | 117.19 | 0.4297 | 505.0 | 475.3 | |
| 1.12 | -3.00 | 0.61 | -3.00 | -8.60 | 323.14 | -22.71 | 117.62 | 0.4326 | 768.8 | 999999 | |
| 0.00 | 4.05 | 0.00 | 2.23 | -8.52 | 322.85 | -22.99 | 117.15 | 0.4360 | 766.0 | 677.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -9.86 | 322.62 | -23.22 | 119.63 | 0.4488 | 768.0 | 712.4 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -9.71 | 322.60 | -23.24 | 119.31 | 0.4479 | 734.0 | 620.9 | |
| 0.00 | 2.41 | 0.00 | 1.33 | -7.66 | 321.95 | -23.89 | 114.52 | 0.4430 | 759.0 | 661.3 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -9.45 | 321.80 | -24.04 | 117.99 | 0.4571 | 726.0 | 599.4 | |
| 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. | |