SDO HMI 2014-03-05 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.83 | 49.97 | 9.08 | 28.48 | -17.23 | 44.70 | -28.61 | 112.40 | 0.4964 | -198.5 | 142.6 | |
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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 |
| 1.82 | 9.60 | 1.02 | 5.37 | -16.78 | 46.66 | -26.64 | 112.58 | 0.4669 | 1055.2 | 808.4 | |
| 1.64 | 8.47 | 0.92 | 4.76 | -17.15 | 46.29 | -27.02 | 113.12 | 0.4739 | 855.4 | 620.0 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -16.24 | 46.22 | -27.08 | 111.22 | 0.4709 | 734.0 | 609.3 | |
| 0.35 | -2.00 | 0.19 | -2.00 | -17.19 | 45.96 | -27.34 | 113.01 | 0.4786 | 625.5 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -16.28 | 45.97 | -27.33 | 111.18 | 0.4746 | 738.0 | 560.2 | |
| 0.00 | 1.64 | 0.00 | 0.93 | -17.62 | 45.47 | -27.83 | 113.57 | 0.4874 | 587.0 | 523.8 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -17.25 | 45.43 | -27.87 | 112.82 | 0.4864 | -562.0 | -370.7 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -17.40 | 44.87 | -28.43 | 112.80 | 0.4948 | 372.0 | 333.0 | |
| 0.95 | 2.51 | 0.54 | 1.43 | -17.38 | 44.55 | -28.75 | 112.59 | 0.4992 | 593.8 | 495.3 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -17.68 | 44.43 | -28.87 | 113.10 | 0.5021 | -607.0 | -372.5 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -16.35 | 43.98 | -29.32 | 110.30 | 0.5030 | -683.0 | -575.4 | |
| 0.61 | 20.41 | 0.35 | 11.81 | -17.66 | 43.54 | -29.76 | 112.58 | 0.5144 | -869.9 | -674.1 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -16.28 | 43.39 | -29.91 | 109.90 | 0.5112 | -750.0 | -624.2 | |
| 10.46 | -12.00 | 6.06 | -12.00 | -17.54 | 43.06 | -30.25 | 112.11 | 0.5205 | -886.2 | 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. | |