SDO HMI 2014-04-09 06:05:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.19 | 0.00 | 10.56 | -17.13 | 349.89 | 14.86 | 230.99 | 0.3175 | -837.2 | -674.6 | |
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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 |
| 0.00 | 0.71 | 0.00 | 0.38 | -18.51 | 356.18 | 21.14 | 236.96 | 0.4097 | -701.0 | -626.9 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -17.91 | 356.32 | 21.28 | 238.40 | 0.4072 | -811.0 | -646.3 | |
| 0.00 | 1.50 | 0.00 | 0.81 | -21.20 | 352.97 | 17.94 | 227.17 | 0.3932 | -681.0 | -567.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -17.64 | 356.12 | 21.08 | 238.79 | 0.4025 | -847.0 | -662.1 | |
| 0.00 | 2.82 | 0.00 | 1.47 | -17.25 | 349.32 | 14.29 | 230.04 | 0.3088 | -813.0 | -656.1 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -16.53 | 349.79 | 14.76 | 232.81 | 0.3079 | -740.0 | -596.0 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -16.80 | 349.45 | 14.41 | 231.47 | 0.3059 | -1071.0 | -857.7 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -16.93 | 349.28 | 14.24 | 230.80 | 0.3050 | -869.0 | -787.5 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -16.53 | 349.61 | 14.57 | 232.48 | 0.3055 | -806.0 | -599.6 | |
| 0.00 | 2.20 | 0.00 | 1.14 | -14.35 | 349.84 | 14.80 | 239.16 | 0.2896 | -886.0 | -705.6 | |
| 0.00 | 2.29 | 0.00 | 1.18 | -19.83 | 344.51 | 9.47 | 212.87 | 0.2865 | -939.0 | -540.9 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -17.99 | 345.36 | 10.32 | 219.26 | 0.2705 | -762.0 | -656.9 | |
| 0.00 | 2.56 | 0.00 | 1.31 | -13.86 | 348.68 | 13.65 | 238.76 | 0.2691 | -958.0 | -805.3 | |
| 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. | |