SDO HMI 2014-10-31 05:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.14 | 50.10 | 7.66 | 38.46 | -16.18 | 100.44 | -45.81 | 115.63 | 0.7652 | 360.4 | 370.7 | |
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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 |
| 0.52 | 24.70 | 0.39 | 18.47 | -16.12 | 101.85 | -44.40 | 116.17 | 0.7512 | 843.0 | 580.8 | |
| 3.55 | -1.00 | 2.65 | -1.00 | -15.87 | 101.79 | -44.46 | 115.84 | 0.7508 | 928.2 | 999999 | |
| 0.00 | 2.60 | 0.00 | 1.95 | -15.76 | 101.48 | -44.77 | 115.55 | 0.7537 | 468.0 | 388.7 | |
| 0.61 | -1.00 | 0.46 | -1.00 | -15.60 | 101.48 | -44.77 | 115.36 | 0.7530 | 603.7 | 999999 | |
| 3.55 | 13.78 | 2.70 | 10.51 | -16.08 | 100.85 | -45.40 | 115.67 | 0.7613 | 752.7 | 515.0 | |
| 1.91 | -5.00 | 1.46 | -5.00 | -16.13 | 100.57 | -45.68 | 115.60 | 0.7644 | 498.9 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.59 | -15.17 | 100.18 | -46.07 | 114.26 | 0.7646 | 629.0 | 485.3 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -15.37 | 99.50 | -46.75 | 114.21 | 0.7724 | 336.0 | 311.3 | |
| 0.00 | 0.87 | 0.00 | 0.68 | -16.06 | 99.01 | -47.24 | 114.85 | 0.7798 | 517.0 | 395.2 | |
| 0.00 | 0.69 | 0.00 | 0.55 | -15.96 | 98.59 | -47.67 | 114.55 | 0.7837 | -341.0 | -366.2 | |
| 0.00 | 1.13 | 0.00 | 0.92 | -16.20 | 97.24 | -49.01 | 114.30 | 0.7976 | -523.0 | -434.7 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -16.54 | 95.18 | -51.07 | 113.93 | 0.8181 | -455.0 | -386.0 | |
| 0.00 | 1.65 | 0.00 | 1.49 | -19.12 | 93.80 | -52.45 | 116.38 | 0.8383 | -639.0 | -567.5 | |
| 0.00 | 2.08 | 0.00 | 1.88 | -18.80 | 93.74 | -52.51 | 116.00 | 0.8378 | -540.0 | -466.1 | |
| 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. | |