SDO HMI 2014-05-27 10:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 20.37 | 0.19 | 10.90 | -20.38 | 48.30 | -10.18 | 154.33 | 0.3719 | 185.2 | 100.5 | |
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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 | 1.08 | 0.00 | 0.57 | -18.69 | 52.78 | -5.70 | 162.59 | 0.3159 | 773.0 | 587.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -19.01 | 52.51 | -5.97 | 162.15 | 0.3222 | 745.0 | 585.5 | |
| 0.00 | 2.98 | 0.00 | 1.56 | -18.72 | 52.36 | -6.12 | 161.43 | 0.3185 | 906.0 | 680.0 | |
| 0.36 | 1.89 | 0.19 | 0.99 | -19.19 | 51.40 | -7.08 | 159.34 | 0.3312 | 907.0 | 789.9 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -20.09 | 50.67 | -7.80 | 158.48 | 0.3491 | 700.0 | 551.1 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -20.15 | 50.44 | -8.04 | 157.98 | 0.3515 | 906.0 | 757.9 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -21.28 | 49.79 | -8.69 | 157.68 | 0.3724 | 856.0 | 667.6 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -20.21 | 49.85 | -8.63 | 156.61 | 0.3562 | 773.0 | 581.5 | |
| 0.00 | 1.99 | 0.00 | 1.05 | -19.57 | 49.53 | -8.95 | 155.04 | 0.3489 | -983.0 | -837.4 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -21.76 | 42.79 | -15.69 | 144.45 | 0.4337 | -769.0 | -621.5 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -21.89 | 42.54 | -15.94 | 144.22 | 0.4376 | -890.0 | -725.8 | |
| 0.00 | 1.71 | 0.00 | 0.95 | -22.21 | 42.09 | -16.39 | 143.95 | 0.4457 | -854.0 | -652.9 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -22.40 | 41.83 | -16.65 | 143.80 | 0.4504 | -800.0 | -616.2 | |
| 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. | |