SDO HMI 2014-03-31 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.17 | 0.00 | 12.04 | -27.18 | 84.05 | -7.05 | 168.16 | 0.3959 | -61.4 | -3.7 | |
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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 | 2.46 | 0.00 | 1.28 | -23.50 | 98.09 | 6.99 | 200.93 | 0.3140 | 738.0 | 630.2 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -22.80 | 96.07 | 4.97 | 195.91 | 0.2924 | 870.0 | 727.2 | |
| 0.00 | 1.58 | 0.00 | 0.81 | -21.87 | 95.68 | 4.58 | 195.66 | 0.2756 | 812.0 | 636.7 | |
| 0.00 | 1.40 | 0.00 | 0.74 | -26.25 | 92.65 | 1.55 | 184.13 | 0.3392 | 717.0 | 467.5 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -23.85 | 91.55 | 0.45 | 181.38 | 0.2985 | 915.0 | 738.0 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -27.15 | 90.65 | -0.45 | 178.85 | 0.3530 | 580.0 | 473.6 | |
| 0.00 | 2.98 | 0.00 | 1.58 | -26.89 | 90.48 | -0.62 | 178.41 | 0.3489 | 873.0 | 564.5 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -26.60 | 81.19 | -9.91 | 155.89 | 0.3785 | -744.0 | -638.8 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -29.24 | 79.99 | -11.11 | 156.54 | 0.4240 | -967.0 | -764.3 | |
| 0.00 | 0.26 | 0.00 | 0.15 | -29.32 | 77.59 | -13.51 | 152.39 | 0.4413 | -785.0 | -642.3 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -34.17 | 76.58 | -14.52 | 156.02 | 0.5125 | -526.0 | -490.7 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -28.06 | 76.61 | -14.49 | 149.13 | 0.4323 | -752.0 | -597.6 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -29.06 | 76.36 | -14.74 | 150.03 | 0.4472 | -994.0 | -829.1 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -26.66 | 76.00 | -15.10 | 146.14 | 0.4197 | -462.0 | -424.4 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -33.06 | 72.37 | -18.73 | 149.18 | 0.5274 | -665.0 | -455.0 | |
| 0.00 | 2.19 | 0.00 | 1.31 | -29.77 | 65.14 | -25.96 | 136.75 | 0.5567 | -592.0 | -545.7 | |
| 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. | |