SDO HMI 2014-09-05 06:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.54 | 0.00 | 10.75 | 10.04 | 180.28 | 15.62 | 249.86 | 0.2899 | -66.0 | -169.7 | |
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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 |
| 0.00 | 0.98 | 0.00 | 0.53 | 3.89 | 188.12 | 23.45 | 263.10 | 0.4016 | -479.0 | -413.3 | |
| 0.00 | 1.70 | 0.00 | 0.91 | 6.85 | 187.61 | 22.94 | 270.46 | 0.3887 | -789.0 | -702.5 | |
| 0.00 | 1.43 | 0.00 | 0.77 | 11.45 | 187.90 | 23.23 | 282.16 | 0.3972 | -763.0 | -601.4 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 11.25 | 187.58 | 22.91 | 281.78 | 0.3918 | -778.0 | -628.8 | |
| 0.00 | 2.77 | 0.00 | 1.49 | 11.61 | 187.04 | 22.38 | 282.91 | 0.3842 | -780.0 | -626.1 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 11.75 | 186.69 | 22.02 | 283.42 | 0.3790 | -697.0 | -564.0 | |
| 0.00 | 3.13 | 0.00 | 1.67 | 11.86 | 186.23 | 21.57 | 283.92 | 0.3722 | -806.0 | -668.5 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 11.26 | 186.05 | 21.38 | 282.40 | 0.3677 | -812.0 | -622.6 | |
| 0.00 | 0.89 | 0.00 | 0.46 | 11.27 | 177.81 | 13.14 | 288.24 | 0.2358 | 842.0 | 642.5 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 9.47 | 171.84 | 7.18 | 287.92 | 0.1301 | 811.0 | 625.2 | |
| 0.00 | 2.15 | 0.00 | 1.07 | 2.97 | 169.31 | 4.65 | 227.54 | 0.1102 | 957.0 | 670.8 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 12.10 | 166.23 | 1.57 | 342.48 | 0.0893 | 814.0 | 628.9 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 11.68 | 164.13 | -0.53 | 6.71 | 0.0784 | 805.0 | 598.0 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 16.49 | 161.10 | -3.57 | 20.34 | 0.1724 | 751.0 | 568.0 | |
| 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. | |