SDO HMI 2014-04-08 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.03 | 0.00 | 9.78 | -18.33 | 349.73 | -0.74 | 176.70 | 0.2435 | -422.2 | -347.0 | |
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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 | 1.41 | 0.00 | 0.77 | -23.33 | 9.58 | 19.11 | 224.96 | 0.4272 | 824.0 | 681.9 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -17.10 | 2.37 | 11.89 | 225.68 | 0.2766 | 658.0 | 481.2 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -17.87 | 355.68 | 5.21 | 202.99 | 0.2224 | -809.0 | -710.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -12.41 | 355.00 | 4.53 | 215.17 | 0.1346 | -643.0 | -434.7 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -23.44 | 353.90 | 3.43 | 190.46 | 0.3039 | -807.0 | -667.7 | |
| 0.00 | 1.15 | 0.00 | 0.57 | -9.50 | 350.18 | -0.29 | 175.12 | 0.0591 | -839.0 | -644.4 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -15.87 | 349.64 | -0.84 | 175.25 | 0.1704 | -857.0 | -647.4 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -17.37 | 349.53 | -0.94 | 175.41 | 0.1963 | -530.0 | -467.8 | |
| 0.00 | 1.85 | 0.00 | 0.93 | -13.83 | 348.81 | -1.66 | 168.14 | 0.1375 | -757.0 | -700.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.03 | 348.75 | -1.72 | 171.36 | 0.1920 | -778.0 | -540.0 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -15.83 | 346.73 | -3.74 | 159.58 | 0.1806 | -794.0 | -647.4 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -17.70 | 345.18 | -5.30 | 156.37 | 0.2203 | -768.0 | -634.9 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -25.38 | 343.34 | -7.13 | 161.24 | 0.3504 | 27.0 | 8.9 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -24.56 | 341.29 | -9.18 | 155.41 | 0.3503 | -15.0 | -9.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -19.56 | 339.87 | -10.60 | 143.45 | 0.2924 | -666.0 | -568.8 | |
| 0.00 | 2.03 | 0.00 | 1.07 | -22.18 | 337.46 | -13.01 | 143.22 | 0.3497 | -1.0 | -0.4 | |
| 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. | |