SDO HMI 2014-10-12 01:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.08 | 0.00 | 10.16 | 13.31 | 58.81 | 19.77 | 292.41 | 0.3583 | 44.2 | 76.5 | |
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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 | 1.31 | 0.00 | 0.74 | 12.02 | 66.56 | 27.52 | 284.24 | 0.4682 | -730.0 | -616.7 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 16.31 | 64.17 | 25.14 | 294.62 | 0.4503 | -634.0 | -419.3 | |
| 0.00 | 2.63 | 0.00 | 1.42 | 8.49 | 62.77 | 23.73 | 277.23 | 0.4030 | -795.0 | -649.9 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 18.29 | 60.79 | 21.75 | 301.81 | 0.4157 | -771.0 | -574.7 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 18.58 | 60.59 | 21.55 | 302.63 | 0.4152 | -619.0 | -517.4 | |
| 0.00 | 2.80 | 0.00 | 1.49 | 12.73 | 59.84 | 20.80 | 289.42 | 0.3689 | 831.0 | 678.9 | |
| 0.00 | 1.84 | 0.00 | 0.98 | 15.76 | 58.95 | 19.91 | 297.95 | 0.3726 | -852.0 | -692.4 | |
| 0.00 | 2.98 | 0.00 | 1.55 | 13.64 | 55.28 | 16.24 | 296.46 | 0.3049 | 606.0 | 643.1 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 13.13 | 55.18 | 16.14 | 295.03 | 0.3001 | 827.0 | 594.7 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 13.36 | 54.65 | 15.61 | 296.42 | 0.2936 | 908.0 | 769.7 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 13.25 | 54.13 | 15.09 | 296.79 | 0.2852 | 822.0 | 695.5 | |
| 0.00 | 1.66 | 0.00 | 0.85 | 11.85 | 51.21 | 12.18 | 296.39 | 0.2315 | 938.0 | 734.0 | |
| 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. | |