SDO HMI 2014-04-10 12:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.72 | 0.00 | 13.82 | -13.22 | 305.09 | -13.50 | 117.30 | 0.2778 | 321.2 | 406.8 | |
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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 | 1.50 | 0.00 | 0.76 | -14.80 | 310.86 | -7.74 | 139.93 | 0.2031 | 946.0 | 827.1 | |
| 0.00 | 2.29 | 0.00 | 1.16 | -13.95 | 310.77 | -7.83 | 136.65 | 0.1935 | 746.0 | 636.5 | |
| 0.00 | 1.76 | 0.00 | 0.90 | -18.05 | 309.61 | -8.99 | 144.82 | 0.2590 | 884.0 | 655.4 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -20.44 | 308.98 | -9.61 | 148.13 | 0.2977 | 811.0 | 549.6 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -0.05 | 309.41 | -9.19 | 57.55 | 0.1901 | 816.0 | 691.9 | |
| 0.00 | 1.59 | 0.00 | 0.81 | -11.57 | 306.74 | -11.86 | 116.44 | 0.2259 | 889.0 | 698.8 | |
| 0.00 | 7.14 | 0.00 | 3.63 | -6.86 | 305.91 | -12.68 | 94.82 | 0.2198 | 966.0 | 778.2 | |
| 0.00 | 1.68 | 0.00 | 0.88 | -19.82 | 304.42 | -14.17 | 136.49 | 0.3361 | 771.0 | 511.3 | |
| 0.00 | 3.26 | 0.00 | 1.74 | -20.54 | 302.32 | -16.27 | 134.27 | 0.3680 | 497.0 | 498.0 | |
| 0.00 | 2.03 | 0.00 | 1.05 | -11.14 | 301.66 | -16.93 | 108.36 | 0.3024 | -953.0 | -661.7 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -16.40 | 296.57 | -22.03 | 117.66 | 0.4080 | -780.0 | -647.4 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -16.66 | 296.26 | -22.33 | 117.97 | 0.4139 | -705.0 | -634.6 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -16.74 | 296.05 | -22.55 | 117.95 | 0.4174 | -712.0 | -583.7 | |
| 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. | |