SDO HMI 2014-03-25 09:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.95 | 45.90 | 9.06 | 27.71 | 3.06 | 137.93 | -33.39 | 74.39 | 0.5726 | 14.6 | -121.5 | |
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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 |
| 3.15 | 6.82 | 1.85 | 4.01 | 3.72 | 140.41 | -30.92 | 71.99 | 0.5413 | -929.6 | -711.2 | |
| 1.31 | 4.72 | 0.77 | 2.78 | 3.25 | 140.22 | -31.11 | 72.94 | 0.5418 | -832.5 | -744.6 | |
| 0.00 | 0.52 | 0.00 | 0.31 | 3.53 | 140.07 | -31.26 | 72.53 | 0.5452 | -554.0 | -473.5 | |
| 0.00 | 3.76 | 0.00 | 2.22 | 2.91 | 139.88 | -31.45 | 73.73 | 0.5450 | -789.0 | -760.7 | |
| 0.00 | 0.61 | 0.00 | 0.36 | 3.24 | 139.86 | -31.46 | 73.15 | 0.5467 | -529.0 | -461.4 | |
| 0.00 | 1.84 | 0.00 | 1.09 | 3.01 | 139.70 | -31.63 | 73.65 | 0.5480 | -443.0 | -385.4 | |
| 1.92 | 3.85 | 1.14 | 2.28 | 3.75 | 139.53 | -31.80 | 72.46 | 0.5536 | -815.0 | -633.6 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 2.59 | 138.79 | -32.54 | 74.86 | 0.5588 | 625.0 | 545.5 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 5.11 | 138.32 | -33.01 | 70.87 | 0.5765 | -738.0 | -617.6 | |
| 1.49 | 2.80 | 0.90 | 1.69 | 3.64 | 138.00 | -33.33 | 73.48 | 0.5741 | 769.9 | 587.4 | |
| 0.00 | 1.92 | 0.00 | 1.17 | 5.48 | 137.87 | -33.46 | 70.54 | 0.5843 | -434.0 | -425.8 | |
| 0.00 | 1.31 | 0.00 | 0.81 | 1.58 | 135.85 | -35.48 | 77.89 | 0.5957 | 681.0 | 579.1 | |
| 0.00 | 3.06 | 0.00 | 1.89 | 2.53 | 135.60 | -35.73 | 76.44 | 0.6024 | 875.0 | 700.8 | |
| 7.08 | 11.63 | 4.40 | 7.23 | 2.17 | 135.17 | -36.16 | 77.20 | 0.6069 | 833.8 | 626.6 | |
| 0.00 | 1.22 | 0.00 | 0.76 | 2.45 | 135.08 | -36.25 | 76.79 | 0.6090 | 512.0 | 426.6 | |
| 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. | |