SDO HMI 2014-10-02 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.65 | 0.00 | 14.92 | -5.35 | 138.80 | -25.06 | 115.03 | 0.4675 | -650.8 | -604.4 | |
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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 | 1.41 | 0.00 | 0.78 | -5.26 | 140.44 | -23.41 | 116.44 | 0.4437 | -738.0 | -449.8 | |
| 0.00 | 3.87 | 0.00 | 2.14 | -4.55 | 139.81 | -24.04 | 114.39 | 0.4478 | -686.0 | -633.7 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -4.54 | 139.38 | -24.47 | 113.98 | 0.4538 | -615.0 | -525.2 | |
| 0.00 | 1.76 | 0.00 | 0.98 | -5.80 | 139.30 | -24.56 | 116.38 | 0.4635 | -951.0 | -806.2 | |
| 0.00 | 3.78 | 0.00 | 2.11 | -5.53 | 139.18 | -24.68 | 115.74 | 0.4633 | -896.0 | -733.6 | |
| 0.00 | 3.78 | 0.00 | 2.12 | -6.40 | 138.97 | -24.89 | 117.21 | 0.4722 | -753.0 | -632.3 | |
| 0.00 | 3.78 | 0.00 | 2.10 | -3.37 | 139.06 | -24.79 | 111.30 | 0.4512 | -561.0 | -644.2 | |
| 0.00 | 1.41 | 0.00 | 0.79 | -6.13 | 138.95 | -24.91 | 116.67 | 0.4705 | -704.0 | -554.8 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -6.52 | 138.49 | -25.36 | 116.98 | 0.4795 | -701.0 | -571.8 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -7.28 | 138.15 | -25.71 | 118.04 | 0.4895 | -626.0 | -615.2 | |
| 0.00 | 0.35 | 0.00 | 0.20 | -6.54 | 138.12 | -25.73 | 116.67 | 0.4846 | -424.0 | -507.2 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -6.09 | 136.12 | -27.73 | 114.12 | 0.5090 | -683.0 | -622.2 | |
| 0.00 | 1.94 | 0.00 | 1.11 | -4.91 | 135.87 | -27.98 | 111.78 | 0.5054 | -122.0 | -184.2 | |
| 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. | |