SDO HMI 2011-07-04 13:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.60 | 162.67 | 35.82 | 120.64 | 15.48 | 26.54 | 47.32 | 287.99 | 0.7470 | -285.2 | -353.2 | |
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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 |
| 1.73 | 2.27 | 1.34 | 1.77 | 16.72 | 28.72 | 49.50 | 289.12 | 0.7730 | -346.5 | -394.7 | |
| 0.00 | 0.64 | 0.00 | 0.49 | 15.95 | 28.41 | 49.18 | 288.20 | 0.7682 | -562.0 | -460.7 | |
| 0.00 | 0.91 | 0.00 | 0.70 | 16.21 | 28.20 | 48.98 | 288.57 | 0.7665 | -437.0 | -280.0 | |
| 20.44 | 125.07 | 15.37 | 93.47 | 15.40 | 27.22 | 48.00 | 287.73 | 0.7544 | -894.7 | -448.8 | |
| 7.90 | -4.00 | 5.88 | -4.00 | 14.92 | 26.80 | 47.57 | 287.18 | 0.7488 | -896.6 | 999999 | |
| 0.00 | 2.63 | 0.00 | 1.98 | 16.41 | 27.07 | 47.84 | 289.09 | 0.7547 | -525.0 | -481.6 | |
| 0.00 | 2.45 | 0.00 | 1.81 | 16.13 | 26.18 | 46.95 | 288.93 | 0.7444 | 199.0 | 145.6 | |
| 0.00 | 1.18 | 0.00 | 0.85 | 13.69 | 25.44 | 46.21 | 285.81 | 0.7313 | -612.0 | -544.3 | |
| 1.82 | -4.00 | 1.33 | -4.00 | 15.46 | 25.70 | 46.47 | 288.15 | 0.7376 | 423.9 | 999999 | |
| 1.18 | 2.72 | 0.84 | 1.95 | 15.83 | 24.26 | 45.03 | 289.00 | 0.7221 | 490.5 | 405.5 | |
| 13.90 | 19.26 | 9.91 | 13.73 | 16.37 | 24.10 | 44.87 | 289.78 | 0.7216 | 706.9 | 387.8 | |
| 0.00 | 1.27 | 0.00 | 0.90 | 15.88 | 23.73 | 44.50 | 289.21 | 0.7162 | 700.0 | 528.4 | |
| 1.63 | 4.27 | 1.15 | 2.99 | 15.71 | 23.24 | 44.01 | 289.10 | 0.7101 | 709.1 | 650.8 | |
| 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. | |