SDO HMI 2014-09-24 19:02:48 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.33 | 22.90 | 0.75 | 13.10 | -15.50 | 246.53 | -20.11 | 138.56 | 0.5027 | -800.6 | -671.0 | |
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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 | 2.92 | 0.00 | 1.67 | -15.72 | 247.11 | -19.54 | 139.66 | 0.4994 | -912.0 | -696.0 | |
| 0.00 | 1.15 | 0.00 | 0.65 | -14.29 | 247.24 | -19.40 | 137.88 | 0.4819 | -763.0 | -679.2 | |
| 0.00 | 2.12 | 0.00 | 1.21 | -16.01 | 247.04 | -19.60 | 139.97 | 0.5034 | -693.0 | -534.8 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -15.79 | 246.93 | -19.71 | 139.51 | 0.5019 | -882.0 | -733.1 | |
| 0.80 | 3.71 | 0.45 | 2.11 | -15.27 | 246.95 | -19.69 | 138.83 | 0.4959 | -926.6 | -777.3 | |
| 0.00 | 1.06 | 0.00 | 0.61 | -15.96 | 246.72 | -19.93 | 139.43 | 0.5060 | -588.0 | -481.8 | |
| 0.00 | 0.62 | 0.00 | 0.35 | -15.47 | 246.73 | -19.91 | 138.80 | 0.5003 | -631.0 | -517.7 | |
| 0.00 | 1.77 | 0.00 | 1.02 | -15.73 | 246.11 | -20.54 | 138.27 | 0.5094 | -716.0 | -536.7 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -15.18 | 246.07 | -20.58 | 137.46 | 0.5038 | -970.0 | -859.3 | |
| 0.00 | 1.86 | 0.00 | 1.07 | -15.93 | 245.92 | -20.73 | 138.28 | 0.5135 | -697.0 | -539.7 | |
| 0.00 | 2.83 | 0.00 | 1.62 | -15.34 | 245.95 | -20.70 | 137.53 | 0.5068 | -873.0 | -798.2 | |
| 0.00 | 1.15 | 0.00 | 0.66 | -14.99 | 245.95 | -20.69 | 137.04 | 0.5029 | -794.0 | -674.6 | |
| 0.53 | 1.59 | 0.30 | 0.91 | -15.42 | 245.71 | -20.94 | 137.30 | 0.5101 | -881.2 | -736.9 | |
| 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. | |