SDO HMI 2014-10-02 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.66 | 0.00 | 10.20 | -5.28 | 138.85 | -22.25 | 117.73 | 0.4277 | -845.5 | -712.6 | |
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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 | 1.23 | 0.00 | 0.66 | -4.33 | 140.58 | -20.51 | 117.66 | 0.3962 | -859.0 | -608.1 | |
| 0.00 | 1.67 | 0.00 | 0.91 | -4.63 | 139.99 | -21.10 | 117.63 | 0.4068 | -967.0 | -826.1 | |
| 0.00 | 1.76 | 0.00 | 0.95 | -4.49 | 139.68 | -21.42 | 116.96 | 0.4102 | -888.0 | -773.2 | |
| 0.00 | 3.08 | 0.00 | 1.68 | -5.79 | 139.47 | -21.63 | 119.47 | 0.4230 | -989.0 | -848.9 | |
| 0.00 | 1.76 | 0.00 | 0.96 | -5.55 | 139.31 | -21.78 | 118.79 | 0.4232 | -941.0 | -830.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -3.83 | 139.34 | -21.76 | 115.16 | 0.4103 | -951.0 | -787.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -4.51 | 139.29 | -21.81 | 116.57 | 0.4158 | -721.0 | -636.6 | |
| 0.00 | 1.94 | 0.00 | 1.06 | -6.35 | 139.15 | -21.95 | 120.25 | 0.4318 | -804.0 | -679.9 | |
| 0.00 | 1.50 | 0.00 | 0.83 | -6.52 | 138.16 | -22.94 | 119.46 | 0.4465 | -750.0 | -563.9 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -3.47 | 137.20 | -23.90 | 112.29 | 0.4389 | -709.0 | -531.6 | |
| 0.00 | 2.46 | 0.00 | 1.38 | -6.03 | 136.10 | -24.99 | 116.42 | 0.4711 | -722.0 | -586.8 | |
| 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. | |