SDO HMI 2014-09-24 17:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.36 | 0.00 | 11.15 | -15.40 | 246.44 | -21.33 | 136.74 | 0.5138 | -798.0 | -734.6 | |
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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 | 0.80 | 0.00 | 0.46 | -15.80 | 247.16 | -20.61 | 138.26 | 0.5109 | -746.0 | -620.6 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -15.67 | 247.14 | -20.63 | 138.06 | 0.5096 | -851.0 | -680.9 | |
| 0.00 | 1.50 | 0.00 | 0.86 | -15.15 | 247.13 | -20.64 | 137.33 | 0.5041 | -894.0 | -740.5 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -14.57 | 247.12 | -20.65 | 136.50 | 0.4979 | -895.0 | -709.2 | |
| 0.00 | 1.15 | 0.00 | 0.66 | -15.74 | 246.93 | -20.84 | 137.87 | 0.5125 | -820.0 | -719.5 | |
| 0.00 | 2.30 | 0.00 | 1.32 | -15.29 | 246.85 | -20.93 | 137.14 | 0.5085 | -917.0 | -864.2 | |
| 0.00 | 0.62 | 0.00 | 0.36 | -15.72 | 246.73 | -21.04 | 137.57 | 0.5143 | -568.0 | -468.4 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -15.47 | 246.63 | -21.14 | 137.08 | 0.5126 | -677.0 | -564.4 | |
| 0.00 | 2.74 | 0.00 | 1.58 | -15.10 | 246.10 | -21.67 | 135.87 | 0.5142 | -715.0 | -766.8 | |
| 0.00 | 2.21 | 0.00 | 1.28 | -15.92 | 245.87 | -21.90 | 136.71 | 0.5251 | -682.0 | -525.0 | |
| 0.00 | 4.86 | 0.00 | 2.81 | -15.34 | 245.87 | -21.90 | 135.90 | 0.5190 | -1013.0 | -857.8 | |
| 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. | |