SDO HMI 2014-03-29 03:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.54 | 0.00 | 9.43 | -26.59 | 86.26 | -35.60 | 125.79 | 0.6284 | -132.5 | -21.9 | |
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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 | 3.07 | 0.00 | 1.68 | -23.04 | 101.54 | -20.32 | 132.01 | 0.4319 | 727.0 | 726.1 | |
| 0.00 | 0.35 | 0.00 | 0.20 | -23.45 | 98.84 | -23.02 | 129.58 | 0.4675 | 671.0 | 589.5 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -23.03 | 95.26 | -26.60 | 125.36 | 0.5074 | 535.0 | 424.0 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -26.84 | 90.49 | -31.37 | 127.72 | 0.5895 | 774.0 | 629.0 | |
| 0.00 | 1.23 | 0.00 | 0.76 | -26.49 | 88.97 | -32.89 | 126.16 | 0.6042 | 394.0 | 354.6 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -28.61 | 82.76 | -39.10 | 125.57 | 0.6830 | -422.0 | -457.8 | |
| 0.00 | 1.14 | 0.00 | 0.76 | -26.93 | 83.48 | -38.38 | 123.63 | 0.6672 | -589.0 | -413.0 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -28.04 | 82.57 | -39.29 | 124.71 | 0.6821 | -688.0 | -578.3 | |
| 0.00 | 1.66 | 0.00 | 1.14 | -28.28 | 81.80 | -40.06 | 124.66 | 0.6913 | -526.0 | -418.7 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -27.57 | 81.86 | -40.00 | 123.72 | 0.6874 | -551.0 | -498.5 | |
| 0.00 | 0.61 | 0.00 | 0.42 | -27.35 | 81.95 | -39.91 | 123.46 | 0.6854 | -530.0 | -426.9 | |
| 0.00 | 0.61 | 0.00 | 0.47 | -32.17 | 76.42 | -45.43 | 127.29 | 0.7604 | -528.0 | -441.0 | |
| 0.00 | 1.23 | 0.00 | 0.91 | -26.89 | 75.65 | -46.21 | 120.36 | 0.7484 | -712.0 | -566.4 | |
| 0.00 | 0.96 | 0.00 | 0.78 | -28.85 | 71.57 | -50.29 | 121.56 | 0.7930 | -410.0 | -363.6 | |
| 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. | |