SDO HMI 2014-04-16 23:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.51 | 0.00 | 10.26 | -16.43 | 202.22 | -31.09 | 112.27 | 0.5371 | -486.8 | -452.4 | |
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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 | 0.80 | 0.00 | 0.44 | -13.50 | 207.47 | -25.84 | 109.34 | 0.4510 | 774.0 | 664.6 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -14.61 | 206.95 | -26.36 | 111.38 | 0.4633 | 539.0 | 396.9 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -14.87 | 203.24 | -30.07 | 109.92 | 0.5172 | -761.0 | -557.0 | |
| 0.00 | 1.15 | 0.00 | 0.67 | -15.78 | 203.02 | -30.29 | 111.51 | 0.5238 | -714.0 | -568.1 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -15.92 | 202.78 | -30.53 | 111.65 | 0.5277 | -666.0 | -451.5 | |
| 0.00 | 1.77 | 0.00 | 1.04 | -15.94 | 201.97 | -31.34 | 111.29 | 0.5389 | -839.0 | -679.0 | |
| 0.00 | 1.86 | 0.00 | 1.10 | -17.56 | 201.63 | -31.68 | 113.99 | 0.5501 | -710.0 | -611.0 | |
| 0.00 | 1.24 | 0.00 | 0.73 | -15.75 | 201.89 | -31.42 | 110.92 | 0.5392 | -879.0 | -727.2 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -16.06 | 201.80 | -31.51 | 111.42 | 0.5416 | -651.0 | -528.1 | |
| 0.00 | 3.89 | 0.00 | 2.31 | -17.76 | 201.33 | -31.98 | 114.18 | 0.5550 | -502.0 | -478.9 | |
| 0.00 | 1.42 | 0.00 | 0.84 | -17.68 | 201.01 | -32.30 | 113.88 | 0.5589 | -588.0 | -426.6 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -15.79 | 201.30 | -32.01 | 110.71 | 0.5474 | -622.0 | -505.4 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -16.30 | 200.53 | -32.78 | 111.27 | 0.5597 | -710.0 | -549.0 | |
| 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. | |