SDO HMI 2014-06-05 07:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.93 | 0.00 | 10.76 | 3.37 | 271.72 | -29.31 | 82.83 | 0.4949 | -734.6 | -652.5 | |
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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 | 0.90 | 0.00 | 0.51 | 8.16 | 273.11 | -27.91 | 72.69 | 0.4873 | -656.0 | -562.5 | |
| 0.00 | 2.53 | 0.00 | 1.42 | 3.69 | 273.04 | -27.98 | 81.87 | 0.4749 | -868.0 | -756.5 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 3.05 | 272.96 | -28.07 | 83.24 | 0.4751 | -790.0 | -593.7 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 3.45 | 272.88 | -28.15 | 82.42 | 0.4770 | -858.0 | -734.6 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 3.27 | 272.64 | -28.39 | 82.86 | 0.4803 | -805.0 | -708.2 | |
| 0.00 | 1.90 | 0.00 | 1.08 | 4.49 | 272.39 | -28.64 | 80.41 | 0.4865 | -840.0 | -728.3 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -0.17 | 272.30 | -28.72 | 90.07 | 0.4825 | -712.0 | -560.0 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 3.45 | 270.99 | -30.04 | 82.85 | 0.5055 | -676.0 | -552.5 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 3.70 | 270.63 | -30.40 | 82.45 | 0.5114 | -470.0 | -470.6 | |
| 0.00 | 3.44 | 0.00 | 1.98 | 3.24 | 270.36 | -30.67 | 83.39 | 0.5146 | -714.0 | -716.6 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 3.64 | 270.31 | -30.71 | 82.64 | 0.5160 | -697.0 | -558.0 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 2.48 | 269.49 | -31.53 | 85.00 | 0.5266 | -729.0 | -603.2 | |
| 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. | |