SDO HMI 2014-03-06 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.82 | 130.04 | 29.64 | 145.23 | -9.94 | 359.50 | -64.46 | 97.53 | 0.8981 | 577.3 | 247.8 | |
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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 |
| 11.25 | 104.77 | 12.36 | 114.74 | -10.42 | 359.96 | -63.99 | 98.05 | 0.8946 | 853.8 | 351.9 | |
| 11.33 | -1.00 | 12.39 | -1.00 | -9.51 | 0.16 | -63.80 | 97.01 | 0.8935 | 805.7 | 999999 | |
| 2.16 | -1.00 | 2.38 | -1.00 | -10.09 | 359.95 | -64.01 | 97.67 | 0.8948 | 710.3 | 999999 | |
| 0.00 | 3.37 | 0.00 | 3.72 | -8.17 | 0.04 | -63.92 | 95.52 | 0.8951 | -433.0 | -363.8 | |
| 0.00 | 0.43 | 0.00 | 0.49 | -10.16 | 359.22 | -64.74 | 97.79 | 0.9003 | -231.0 | -246.0 | |
| 1.04 | 2.08 | 1.23 | 2.45 | -10.79 | 357.85 | -66.10 | 98.57 | 0.9100 | 167.2 | 240.2 | |
| 0.00 | 1.90 | 0.00 | 2.26 | -9.70 | 357.92 | -66.03 | 97.38 | 0.9100 | 364.0 | 294.1 | |
| 0.00 | 0.61 | 0.00 | 0.72 | -9.25 | 357.95 | -66.01 | 96.88 | 0.9100 | 155.0 | 200.9 | |
| 0.00 | 1.82 | 0.00 | 2.18 | -8.91 | 357.55 | -66.41 | 96.53 | 0.9130 | 551.0 | 450.0 | |
| 0.00 | 3.89 | 0.00 | 4.71 | -9.01 | 357.43 | -66.52 | 96.66 | 0.9138 | 181.0 | 197.9 | |
| 1.04 | 8.74 | 1.28 | 10.76 | -10.22 | 356.87 | -67.09 | 98.01 | 0.9171 | -576.7 | -289.0 | |
| 0.00 | 0.87 | 0.00 | 1.22 | -14.32 | 353.41 | -70.54 | 102.62 | 0.9377 | -194.0 | -236.1 | |
| 0.00 | 1.56 | 0.00 | 1.98 | -9.55 | 356.04 | -67.92 | 97.34 | 0.9230 | -359.0 | -352.4 | |
| 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. | |