SDO HMI 2014-03-30 01:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.15 | 0.00 | 11.83 | -15.52 | 126.27 | 16.50 | 233.05 | 0.3615 | 374.8 | 185.8 | |
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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 | 1.40 | 0.00 | 0.80 | -6.79 | 140.29 | 30.52 | 267.94 | 0.5067 | 720.0 | 667.8 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -9.43 | 138.20 | 28.43 | 262.48 | 0.4757 | 555.0 | 341.3 | |
| 0.00 | 1.75 | 0.00 | 0.96 | -8.76 | 135.52 | 25.75 | 263.65 | 0.4339 | 594.0 | 549.0 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -12.59 | 132.66 | 22.90 | 253.56 | 0.3976 | 608.0 | 501.9 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -13.77 | 132.58 | 22.81 | 250.63 | 0.4009 | 622.0 | 516.8 | |
| 0.00 | 2.19 | 0.00 | 1.18 | -14.04 | 132.51 | 22.74 | 249.92 | 0.4010 | 815.0 | 720.2 | |
| 0.00 | 1.40 | 0.00 | 0.77 | -19.18 | 132.84 | 23.08 | 238.67 | 0.4352 | 859.0 | 732.1 | |
| 0.00 | 2.19 | 0.00 | 1.18 | -15.49 | 131.86 | 22.09 | 245.96 | 0.3985 | 714.0 | 478.9 | |
| 0.00 | 1.40 | 0.00 | 0.75 | -15.54 | 130.76 | 20.99 | 244.91 | 0.3828 | 837.0 | 753.1 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -16.89 | 124.92 | 15.15 | 234.05 | 0.3102 | 739.0 | 564.0 | |
| 0.00 | 4.29 | 0.00 | 2.16 | -15.24 | 116.10 | 6.33 | 215.39 | 0.1846 | -657.0 | -647.1 | |
| 0.00 | 1.75 | 0.00 | 0.91 | -24.00 | 108.63 | -1.13 | 176.53 | 0.2999 | -795.0 | -618.1 | |
| 0.00 | 1.66 | 0.00 | 0.89 | -27.83 | 106.08 | -3.68 | 171.06 | 0.3672 | -738.0 | -566.7 | |
| 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. | |