SDO HMI 2014-04-10 03:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.11 | 0.00 | 9.38 | -15.00 | 300.45 | -23.07 | 113.61 | 0.4137 | -268.9 | -287.5 | |
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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 | 2.38 | 0.00 | 1.20 | -11.41 | 313.36 | -10.17 | 119.03 | 0.1988 | 829.0 | 637.3 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -8.93 | 312.51 | -11.01 | 105.70 | 0.1969 | 686.0 | 540.6 | |
| 0.00 | 0.62 | 0.00 | 0.32 | -5.42 | 309.23 | -14.29 | 88.43 | 0.2469 | 754.0 | 601.7 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -20.64 | 302.33 | -21.20 | 127.47 | 0.4282 | 864.0 | 675.0 | |
| 0.00 | 1.68 | 0.00 | 0.92 | -16.46 | 300.47 | -23.05 | 116.80 | 0.4225 | -747.0 | -699.7 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -15.67 | 300.43 | -23.09 | 114.99 | 0.4184 | -917.0 | -764.9 | |
| 0.00 | 1.76 | 0.00 | 1.00 | -16.68 | 296.35 | -27.17 | 114.18 | 0.4815 | -741.0 | -594.2 | |
| 0.00 | 2.03 | 0.00 | 1.14 | -16.34 | 296.26 | -27.26 | 113.45 | 0.4811 | -795.0 | -637.0 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -14.37 | 296.02 | -27.50 | 109.35 | 0.4761 | -776.0 | -568.1 | |
| 0.00 | 1.15 | 0.00 | 0.65 | -16.86 | 295.65 | -27.87 | 114.09 | 0.4921 | -578.0 | -516.0 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -16.65 | 295.68 | -27.84 | 113.70 | 0.4906 | -657.0 | -516.2 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -11.86 | 296.15 | -27.37 | 104.17 | 0.4659 | -806.0 | -721.8 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -19.42 | 292.03 | -31.49 | 116.60 | 0.5531 | -612.0 | -519.9 | |
| 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. | |