SDO HMI 2014-09-13 11:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.91 | 100.10 | 13.61 | 54.67 | -15.86 | 65.96 | 9.68 | 202.54 | 0.4247 | 775.4 | 549.4 | |
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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 | 1.87 | 0.00 | 1.03 | -16.34 | 67.54 | 11.26 | 205.24 | 0.4411 | 810.0 | 630.6 | |
| 3.29 | 4.63 | 1.81 | 2.54 | -15.93 | 66.94 | 10.66 | 204.46 | 0.4314 | 863.4 | 672.0 | |
| 0.00 | 1.51 | 0.00 | 0.83 | -16.19 | 66.89 | 10.61 | 204.10 | 0.4348 | 679.0 | 562.2 | |
| 0.00 | 1.69 | 0.00 | 0.93 | -16.39 | 66.84 | 10.56 | 203.81 | 0.4373 | 669.0 | 568.5 | |
| 3.29 | 82.13 | 1.80 | 44.78 | -15.86 | 66.59 | 10.31 | 203.81 | 0.4280 | 917.6 | 595.3 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -16.51 | 66.40 | 10.12 | 202.80 | 0.4363 | 668.0 | 493.2 | |
| 6.32 | -5.00 | 3.45 | -5.00 | -15.75 | 66.26 | 9.98 | 203.25 | 0.4244 | 999.3 | 999999 | |
| 4.36 | -5.00 | 2.38 | -5.00 | -15.62 | 66.06 | 9.78 | 202.96 | 0.4213 | 1122.4 | 999999 | |
| 7.65 | -5.00 | 4.17 | -5.00 | -15.51 | 65.84 | 9.56 | 202.58 | 0.4184 | 1229.1 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.73 | -15.94 | 65.73 | 9.45 | 201.96 | 0.4239 | 557.0 | 549.2 | |
| 0.00 | 1.16 | 0.00 | 0.63 | -16.25 | 64.92 | 8.64 | 199.97 | 0.4239 | 700.0 | 684.2 | |
| 0.00 | 1.42 | 0.00 | 0.78 | -16.82 | 62.02 | 5.74 | 193.24 | 0.4196 | -791.0 | -589.9 | |
| 0.00 | 1.33 | 0.00 | 0.73 | -16.92 | 61.80 | 5.52 | 192.70 | 0.4203 | -906.0 | -644.7 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -20.54 | 61.33 | 5.05 | 190.06 | 0.4744 | 715.0 | 491.5 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -21.77 | 57.80 | 1.51 | 182.90 | 0.4872 | 748.0 | 594.7 | |
| 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. | |