SDO HMI 2014-03-20 23:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.33 | 234.42 | 55.90 | 234.27 | -13.49 | 168.50 | -61.06 | 101.58 | 0.8701 | 555.0 | 198.3 | |
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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 |
| 21.09 | 144.22 | 20.14 | 138.17 | -14.55 | 170.09 | -59.47 | 102.78 | 0.8569 | 880.8 | 292.4 | |
| 8.10 | -1.00 | 7.91 | -1.00 | -14.47 | 169.32 | -60.23 | 102.68 | 0.8636 | 300.3 | 999999 | |
| 0.00 | 1.13 | 0.00 | 1.13 | -15.11 | 168.70 | -60.85 | 103.41 | 0.8689 | 282.0 | 225.7 | |
| 0.00 | 2.00 | 0.00 | 2.00 | -13.93 | 168.55 | -61.00 | 102.05 | 0.8701 | 164.0 | 55.5 | |
| 0.00 | 1.05 | 0.00 | 1.03 | -11.46 | 169.18 | -60.38 | 99.19 | 0.8651 | 451.0 | 402.7 | |
| 20.13 | 62.74 | 20.81 | 64.99 | -12.07 | 167.41 | -62.15 | 99.94 | 0.8797 | 614.6 | 111.5 | |
| 1.13 | 9.59 | 1.27 | 10.79 | -12.58 | 164.83 | -64.72 | 100.59 | 0.8997 | -621.2 | -447.4 | |
| 0.00 | 0.26 | 0.00 | 0.30 | -12.77 | 164.67 | -64.89 | 100.82 | 0.9009 | -286.0 | -269.0 | |
| 0.00 | 0.96 | 0.00 | 1.09 | -10.54 | 164.57 | -64.98 | 98.34 | 0.9022 | 318.0 | 288.1 | |
| 0.00 | 1.05 | 0.00 | 1.19 | -10.24 | 164.62 | -64.93 | 98.01 | 0.9020 | 598.0 | 543.6 | |
| 0.44 | 1.74 | 0.50 | 2.00 | -9.88 | 164.40 | -65.16 | 97.62 | 0.9038 | 491.4 | 466.1 | |
| 0.00 | 0.44 | 0.00 | 0.50 | -9.90 | 164.31 | -65.24 | 97.65 | 0.9044 | 512.0 | 563.0 | |
| 3.92 | 6.97 | 4.56 | 8.12 | -10.20 | 163.98 | -65.58 | 98.00 | 0.9067 | 254.6 | 66.7 | |
| 0.00 | 0.70 | 0.00 | 0.82 | -9.31 | 163.65 | -65.90 | 97.04 | 0.9095 | 286.0 | 208.1 | |
| 0.52 | 1.57 | 0.71 | 2.14 | -15.76 | 159.74 | -69.81 | 104.22 | 0.9334 | -453.2 | -391.7 | |
| 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. | |