SDO HMI 2014-10-11 07:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.26 | 453.20 | 44.36 | 294.96 | -20.50 | 18.14 | -30.80 | 132.16 | 0.6492 | 967.5 | 282.6 | |
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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 | 1.14 | 0.00 | 0.73 | -21.29 | 20.57 | -28.37 | 135.38 | 0.6327 | -628.0 | -494.0 | |
| 0.00 | 1.31 | 0.00 | 0.82 | -18.81 | 20.34 | -28.60 | 132.10 | 0.6130 | 549.0 | 477.2 | |
| 0.00 | 2.10 | 0.00 | 1.31 | -18.35 | 20.32 | -28.63 | 131.48 | 0.6093 | 765.0 | 575.7 | |
| 0.44 | 2.37 | 0.27 | 1.48 | -18.49 | 20.00 | -28.94 | 131.37 | 0.6138 | 810.4 | 708.0 | |
| 1.31 | 430.07 | 0.84 | 280.03 | -20.32 | 19.27 | -29.67 | 132.97 | 0.6367 | 995.1 | 288.4 | |
| 0.00 | 1.23 | 0.00 | 0.78 | -20.02 | 19.30 | -29.64 | 132.63 | 0.6339 | 913.0 | 784.4 | |
| 0.00 | 1.14 | 0.00 | 0.71 | -17.37 | 19.74 | -29.20 | 129.65 | 0.6070 | 694.0 | 558.3 | |
| 2.98 | -5.00 | 1.92 | -5.00 | -20.34 | 18.97 | -29.97 | 132.71 | 0.6398 | 1242.3 | 999999 | |
| 0.00 | 6.22 | 0.00 | 3.92 | -18.53 | 19.34 | -29.60 | 130.79 | 0.6209 | 244.0 | 320.2 | |
| 0.00 | 1.75 | 0.00 | 1.09 | -16.74 | 19.20 | -29.74 | 128.32 | 0.6078 | 317.0 | 319.1 | |
| 63.53 | -5.00 | 41.33 | -5.00 | -20.59 | 18.10 | -30.84 | 132.23 | 0.6504 | 1219.3 | 999999 | |
| 0.00 | 2.80 | 0.00 | 1.81 | -16.76 | 16.08 | -32.86 | 125.66 | 0.6418 | -634.0 | -385.3 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -19.35 | 14.83 | -34.11 | 127.98 | 0.6736 | -440.0 | -290.0 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -24.42 | 10.59 | -38.35 | 130.79 | 0.7485 | -223.0 | -327.7 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -18.01 | 10.77 | -38.17 | 123.39 | 0.7063 | -255.0 | -364.6 | |
| 0.00 | 0.88 | 0.00 | 0.73 | -27.17 | 5.96 | -42.98 | 130.81 | 0.8035 | -449.0 | -370.0 | |
| 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. | |