SDO HMI 2014-09-19 14:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.86 | 27.22 | 3.69 | 16.93 | -20.97 | 310.70 | -24.72 | 139.74 | 0.6056 | -110.0 | -150.7 | |
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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 | 0.59 | -20.85 | 314.97 | -20.45 | 144.73 | 0.5676 | 709.0 | 584.7 | |
| 0.00 | 1.33 | 0.00 | 0.79 | -19.16 | 313.53 | -21.89 | 140.96 | 0.5613 | 692.0 | 527.7 | |
| 0.00 | 2.66 | 0.00 | 1.59 | -18.97 | 313.42 | -22.00 | 140.58 | 0.5602 | 929.0 | 775.4 | |
| 0.00 | 1.24 | 0.00 | 0.74 | -18.72 | 313.11 | -22.31 | 139.89 | 0.5603 | 711.0 | 544.6 | |
| 0.00 | 1.51 | 0.00 | 0.91 | -20.08 | 312.66 | -22.76 | 140.96 | 0.5790 | 791.0 | 600.0 | |
| 0.00 | 0.71 | 0.00 | 0.44 | -21.52 | 310.48 | -24.94 | 140.06 | 0.6133 | -804.0 | -699.0 | |
| 1.24 | 2.13 | 0.78 | 1.34 | -21.70 | 310.26 | -25.16 | 140.03 | 0.6170 | -804.8 | -724.5 | |
| 0.98 | 4.70 | 0.61 | 2.94 | -21.07 | 310.03 | -25.39 | 139.05 | 0.6128 | -830.6 | -580.9 | |
| 0.00 | 2.48 | 0.00 | 1.58 | -22.02 | 309.48 | -25.94 | 139.53 | 0.6271 | -602.0 | -543.6 | |
| 2.66 | 7.80 | 1.68 | 4.94 | -21.65 | 309.48 | -25.94 | 139.12 | 0.6233 | -892.8 | -630.7 | |
| 0.98 | -10.00 | 0.62 | -10.00 | -21.63 | 309.24 | -26.18 | 138.83 | 0.6254 | -727.2 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.79 | -21.81 | 309.09 | -26.33 | 138.88 | 0.6284 | -405.0 | -309.7 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -21.00 | 308.82 | -26.60 | 137.67 | 0.6231 | -332.0 | -390.4 | |
| 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. | |