SDO HMI 2014-04-07 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.69 | 144.02 | 24.14 | 74.50 | 10.14 | 0.76 | 0.38 | 358.60 | 0.2886 | -365.9 | -225.3 | |
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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 | 0.79 | 0.00 | 0.41 | 10.16 | 6.00 | 5.62 | 341.03 | 0.2981 | 795.0 | 628.3 | |
| 0.00 | 1.50 | 0.00 | 0.78 | 10.12 | 5.15 | 4.77 | 343.72 | 0.2931 | -474.0 | -364.9 | |
| 0.53 | 72.49 | 0.27 | 37.47 | 9.80 | 4.29 | 3.91 | 346.28 | 0.2842 | -953.0 | -501.8 | |
| 24.40 | -3.00 | 12.61 | -3.00 | 10.08 | 3.80 | 3.42 | 348.14 | 0.2870 | -1242.1 | 999999 | |
| 0.00 | 1.85 | 0.00 | 0.95 | 8.33 | 3.57 | 3.19 | 347.60 | 0.2574 | -845.0 | -723.0 | |
| 0.88 | 2.73 | 0.46 | 1.41 | 10.48 | 3.29 | 2.91 | 350.13 | 0.2920 | -960.7 | -745.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 12.02 | 2.84 | 2.46 | 352.33 | 0.3163 | -687.0 | -589.2 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 11.77 | 1.46 | 1.08 | 356.57 | 0.3099 | -687.0 | -559.9 | |
| 0.00 | 2.20 | 0.00 | 1.15 | 11.55 | 1.43 | 1.05 | 356.63 | 0.3062 | -816.0 | -640.3 | |
| 0.00 | 2.47 | 0.00 | 1.27 | 9.64 | 357.83 | -2.55 | 9.16 | 0.2772 | 873.0 | 638.7 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 11.25 | 357.11 | -3.27 | 10.59 | 0.3057 | 661.0 | 599.3 | |
| 3.26 | 53.91 | 1.69 | 27.88 | 10.21 | 356.91 | -3.47 | 11.94 | 0.2894 | 952.8 | 106.7 | |
| 12.16 | -12.00 | 6.28 | -12.00 | 9.90 | 356.76 | -3.62 | 12.68 | 0.2848 | 995.5 | 999999 | |
| 5.46 | -12.00 | 2.83 | -12.00 | 10.13 | 356.27 | -4.11 | 14.14 | 0.2904 | -1150.9 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 13.05 | 354.47 | -5.92 | 16.99 | 0.3451 | 687.0 | 559.1 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 13.38 | 353.37 | -7.01 | 19.58 | 0.3559 | 940.0 | 869.2 | |
| 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. | |