SDO HMI 2014-04-01 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.12 | 0.00 | 10.70 | 5.09 | 25.12 | -47.83 | 77.51 | 0.7571 | -264.1 | -221.6 | |
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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 | 1.00 | 2.10 | 27.73 | -45.22 | 80.68 | 0.7212 | -421.0 | -375.9 | |
| 0.00 | 1.14 | 0.00 | 0.83 | 4.24 | 27.18 | -45.77 | 77.95 | 0.7330 | -657.0 | -593.8 | |
| 0.00 | 1.67 | 0.00 | 1.21 | 4.11 | 26.93 | -46.02 | 78.21 | 0.7355 | -610.0 | -587.9 | |
| 0.00 | 1.67 | 0.00 | 1.22 | 4.48 | 26.60 | -46.35 | 77.83 | 0.7403 | -574.0 | -523.1 | |
| 0.00 | 1.05 | 0.00 | 0.77 | 4.27 | 26.48 | -46.47 | 78.13 | 0.7411 | -451.0 | -366.2 | |
| 0.00 | 0.70 | 0.00 | 0.52 | 5.09 | 26.15 | -46.80 | 77.15 | 0.7471 | -469.0 | -328.9 | |
| 0.00 | 1.40 | 0.00 | 1.03 | 3.20 | 26.25 | -46.70 | 79.62 | 0.7411 | -240.0 | -182.8 | |
| 0.00 | 0.88 | 0.00 | 0.65 | 5.41 | 26.03 | -46.92 | 76.78 | 0.7493 | -418.0 | -351.2 | |
| 0.00 | 1.84 | 0.00 | 1.39 | 7.24 | 25.72 | -47.23 | 74.52 | 0.7579 | 217.0 | 221.7 | |
| 0.00 | 0.53 | 0.00 | 0.40 | 5.15 | 25.16 | -47.79 | 77.39 | 0.7582 | -311.0 | -252.7 | |
| 0.00 | 0.61 | 0.00 | 0.56 | 8.81 | 18.04 | -54.92 | 75.01 | 0.8393 | 404.0 | 347.3 | |
| 0.00 | 1.23 | 0.00 | 1.12 | 7.65 | 17.53 | -55.42 | 76.48 | 0.8414 | 361.0 | 284.9 | |
| 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. | |