SDO HMI 2014-10-02 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.27 | 126.13 | 21.27 | 85.39 | 7.13 | 209.95 | 43.36 | 273.32 | 0.6844 | -120.7 | 37.4 | |
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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 | 1.14 | 0.00 | 0.81 | 6.63 | 212.42 | 45.83 | 272.77 | 0.7156 | -570.0 | -471.4 | |
| 0.00 | 1.50 | 0.00 | 1.05 | 6.32 | 212.17 | 45.58 | 272.32 | 0.7127 | -534.0 | -450.0 | |
| 12.42 | 40.34 | 8.72 | 28.29 | 7.65 | 212.08 | 45.48 | 274.19 | 0.7109 | -884.8 | -495.7 | |
| 1.50 | 8.01 | 1.04 | 5.53 | 7.21 | 211.20 | 44.61 | 273.52 | 0.7003 | -818.2 | -758.9 | |
| 0.00 | 0.53 | 0.00 | 0.37 | 6.79 | 211.15 | 44.56 | 272.92 | 0.6999 | -571.0 | -560.2 | |
| 1.85 | 5.99 | 1.27 | 4.11 | 6.55 | 210.78 | 44.19 | 272.55 | 0.6955 | -572.8 | -343.8 | |
| 0.00 | 1.85 | 0.00 | 1.27 | 7.40 | 210.76 | 44.16 | 273.77 | 0.6947 | -600.0 | -602.0 | |
| 0.00 | 1.06 | 0.00 | 0.72 | 6.37 | 210.09 | 43.50 | 272.23 | 0.6869 | -615.0 | -500.0 | |
| 0.00 | 0.53 | 0.00 | 0.36 | 7.72 | 210.21 | 43.62 | 274.20 | 0.6877 | -536.0 | -485.5 | |
| 8.81 | 21.05 | 5.87 | 14.02 | 6.61 | 208.88 | 42.28 | 272.51 | 0.6712 | 662.1 | 495.9 | |
| 2.73 | 32.59 | 1.80 | 21.36 | 6.94 | 208.18 | 41.58 | 272.95 | 0.6620 | 610.5 | 607.0 | |
| 0.70 | -11.00 | 0.46 | -11.00 | 7.11 | 207.87 | 41.28 | 273.20 | 0.6580 | 639.4 | 999999 | |
| 0.00 | 3.70 | 0.00 | 2.41 | 6.22 | 207.34 | 40.74 | 271.80 | 0.6515 | 627.0 | 572.5 | |
| 0.00 | 1.06 | 0.00 | 0.69 | 6.69 | 207.15 | 40.55 | 272.50 | 0.6486 | 753.0 | 631.4 | |
| 3.26 | 6.78 | 2.11 | 4.40 | 7.33 | 207.05 | 40.46 | 273.49 | 0.6471 | 837.1 | 611.7 | |
| 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. | |