SDO HMI 2014-09-19 16:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.91 | 25.52 | 4.32 | 15.73 | -20.97 | 310.51 | -23.81 | 140.77 | 0.5974 | -185.6 | -184.9 | |
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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 | 0.71 | 0.00 | 0.42 | -19.40 | 313.70 | -20.62 | 142.88 | 0.5527 | 584.0 | 540.4 | |
| 0.00 | 2.84 | 0.00 | 1.68 | -18.98 | 313.45 | -20.87 | 142.06 | 0.5501 | 854.0 | 736.4 | |
| 0.00 | 1.24 | 0.00 | 0.73 | -18.69 | 313.18 | -21.14 | 141.36 | 0.5493 | 720.0 | 587.4 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -20.05 | 312.71 | -21.61 | 142.36 | 0.5685 | 654.0 | 595.8 | |
| 0.00 | 0.80 | 0.00 | 0.47 | -18.74 | 312.73 | -21.59 | 140.84 | 0.5540 | 650.0 | 552.8 | |
| 1.15 | 2.66 | 0.72 | 1.65 | -21.71 | 310.27 | -24.05 | 141.28 | 0.6074 | -941.5 | -784.5 | |
| 1.42 | 2.92 | 0.88 | 1.81 | -21.07 | 310.03 | -24.29 | 140.29 | 0.6030 | -868.4 | -670.6 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -22.30 | 309.48 | -24.83 | 141.04 | 0.6203 | -601.0 | -505.6 | |
| 0.00 | 1.51 | 0.00 | 0.95 | -22.06 | 309.46 | -24.86 | 140.75 | 0.6181 | -682.0 | -617.9 | |
| 2.57 | 8.42 | 1.61 | 5.28 | -21.68 | 309.46 | -24.86 | 140.33 | 0.6142 | -889.8 | -653.3 | |
| 0.00 | 1.86 | 0.00 | 1.16 | -21.21 | 309.33 | -24.99 | 139.66 | 0.6106 | -724.0 | -560.3 | |
| 1.77 | -10.00 | 1.11 | -10.00 | -21.59 | 309.19 | -25.13 | 139.93 | 0.6157 | -647.8 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -21.74 | 309.12 | -25.19 | 140.02 | 0.6177 | -333.0 | -380.8 | |
| 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. | |