SDO HMI 2014-10-06 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.80 | 0.00 | 13.52 | -18.25 | 76.22 | -39.78 | 122.95 | 0.7252 | 332.6 | 360.6 | |
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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 | 0.70 | 0.00 | 0.49 | -20.41 | 79.96 | -36.04 | 128.06 | 0.7027 | 546.0 | 487.4 | |
| 0.00 | 2.99 | 0.00 | 2.04 | -18.18 | 79.67 | -36.33 | 125.13 | 0.6907 | 781.0 | 715.0 | |
| 0.00 | 1.14 | 0.00 | 0.76 | -15.66 | 79.97 | -36.04 | 122.13 | 0.6713 | 412.0 | 462.9 | |
| 0.00 | 1.23 | 0.00 | 0.82 | -15.13 | 79.73 | -36.28 | 121.27 | 0.6706 | 748.0 | 672.1 | |
| 0.00 | 1.49 | 0.00 | 1.05 | -16.73 | 77.12 | -38.88 | 121.61 | 0.7082 | 827.0 | 663.1 | |
| 0.00 | 1.32 | 0.00 | 0.96 | -19.52 | 75.78 | -40.22 | 124.15 | 0.7378 | 545.0 | 470.7 | |
| 0.00 | 1.32 | 0.00 | 0.93 | -16.77 | 76.54 | -39.46 | 121.30 | 0.7145 | 502.0 | 412.1 | |
| 0.00 | 1.49 | 0.00 | 1.06 | -16.83 | 76.16 | -39.84 | 121.14 | 0.7188 | 624.0 | 545.9 | |
| 0.00 | 1.14 | 0.00 | 0.84 | -19.41 | 75.06 | -40.94 | 123.58 | 0.7442 | 462.0 | 438.2 | |
| 0.00 | 1.85 | 0.00 | 1.36 | -19.22 | 74.95 | -41.05 | 123.29 | 0.7442 | 367.0 | 336.3 | |
| 0.00 | 0.62 | 0.00 | 0.44 | -16.97 | 75.59 | -40.41 | 120.96 | 0.7254 | 421.0 | 435.1 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -14.50 | 75.08 | -40.92 | 117.57 | 0.7177 | 561.0 | 408.0 | |
| 0.00 | 0.88 | 0.00 | 0.69 | -20.55 | 72.29 | -43.71 | 123.30 | 0.7764 | -483.0 | -401.2 | |
| 0.00 | 0.35 | 0.00 | 0.29 | -23.08 | 71.07 | -44.94 | 125.46 | 0.8000 | -371.0 | -411.5 | |
| 0.00 | 1.76 | 0.00 | 1.39 | -19.97 | 71.34 | -44.66 | 122.11 | 0.7822 | -451.0 | -337.6 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -20.30 | 70.95 | -45.05 | 122.28 | 0.7874 | -170.0 | -304.3 | |
| 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. | |