SDO HMI 2014-04-10 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.28 | 0.00 | 9.08 | -13.56 | 302.87 | -16.82 | 115.96 | 0.3203 | 48.3 | 33.5 | |
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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 | 0.35 | 0.00 | 0.18 | -18.59 | 313.42 | -6.27 | 154.73 | 0.2436 | -422.0 | -492.2 | |
| 0.00 | 1.85 | 0.00 | 0.93 | -11.69 | 310.26 | -9.43 | 122.26 | 0.1906 | 824.0 | 739.7 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -18.04 | 309.61 | -10.08 | 141.72 | 0.2698 | 962.0 | 816.6 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -20.10 | 306.64 | -13.05 | 139.35 | 0.3269 | 802.0 | 661.6 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -11.58 | 306.64 | -13.05 | 114.47 | 0.2442 | 785.0 | 662.0 | |
| 0.00 | 2.47 | 0.00 | 1.26 | -6.87 | 305.92 | -13.77 | 94.58 | 0.2382 | 1045.0 | 894.3 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -20.48 | 302.22 | -17.47 | 132.23 | 0.3815 | 773.0 | 609.8 | |
| 0.00 | 1.85 | 0.00 | 0.97 | -11.11 | 301.67 | -18.02 | 107.35 | 0.3194 | -969.0 | -742.5 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -10.98 | 301.49 | -18.21 | 106.82 | 0.3218 | -702.0 | -583.0 | |
| 0.00 | 1.50 | 0.00 | 0.81 | -14.23 | 298.17 | -21.52 | 112.99 | 0.3879 | -104.0 | -148.6 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -16.39 | 296.54 | -23.15 | 116.63 | 0.4237 | -803.0 | -660.4 | |
| 0.00 | 1.94 | 0.00 | 1.06 | -16.72 | 296.33 | -23.36 | 117.17 | 0.4287 | -749.0 | -637.3 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -17.03 | 295.60 | -24.09 | 117.21 | 0.4407 | -814.0 | -646.3 | |
| 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. | |