SDO HMI 2014-05-27 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.06 | 69.72 | 24.02 | 131.01 | -14.35 | 137.94 | 74.52 | 255.47 | 0.9651 | 188.6 | 151.4 | |
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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 |
| 1.53 | 48.89 | 3.18 | 98.59 | -14.40 | 139.47 | 76.05 | 255.49 | 0.9721 | 80.1 | 221.6 | |
| 0.99 | -1.00 | 2.06 | -1.00 | -14.59 | 139.53 | 76.12 | 255.30 | 0.9724 | 58.7 | 999999 | |
| 1.35 | -1.00 | 2.69 | -1.00 | -14.23 | 138.77 | 75.36 | 255.64 | 0.9692 | 671.1 | 999999 | |
| 0.27 | -1.00 | 0.53 | -1.00 | -14.13 | 138.68 | 75.27 | 255.73 | 0.9688 | 658.7 | 999999 | |
| 3.61 | -1.00 | 7.18 | -1.00 | -14.54 | 138.83 | 75.42 | 255.32 | 0.9695 | 644.6 | 999999 | |
| 0.72 | 2.16 | 1.16 | 3.49 | -13.70 | 135.28 | 71.86 | 256.01 | 0.9528 | -89.8 | -92.3 | |
| 1.53 | 2.89 | 2.39 | 4.49 | -13.46 | 134.60 | 71.19 | 256.22 | 0.9492 | -187.2 | -94.4 | |
| 0.99 | 4.96 | 1.62 | 8.05 | -14.67 | 135.52 | 72.11 | 255.01 | 0.9543 | 304.0 | 192.3 | |
| 1.44 | 3.70 | 2.28 | 5.87 | -14.49 | 134.87 | 71.46 | 255.16 | 0.9510 | -153.2 | 0.2 | |
| 0.00 | 1.62 | 0.00 | 2.46 | -13.41 | 134.08 | 70.67 | 256.25 | 0.9464 | -182.0 | -242.4 | |
| 0.00 | 1.08 | 0.00 | 1.63 | -13.70 | 133.90 | 70.48 | 255.94 | 0.9455 | -368.0 | -315.7 | |
| 0.63 | 2.44 | 0.93 | 3.59 | -13.55 | 133.42 | 70.01 | 256.06 | 0.9427 | -230.4 | -352.1 | |
| 0.00 | 0.99 | 0.00 | 1.45 | -13.83 | 133.25 | 69.83 | 255.75 | 0.9418 | -242.0 | -261.4 | |
| 0.00 | 0.99 | 0.00 | 1.39 | -14.17 | 132.38 | 68.97 | 255.34 | 0.9370 | -458.0 | -419.5 | |
| 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. | |