SDO HMI 2014-09-19 12:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.57 | 30.06 | 4.15 | 18.79 | -20.78 | 310.99 | -25.53 | 138.62 | 0.6109 | -289.0 | -66.4 | |
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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 | 1.24 | 0.00 | 0.75 | -20.87 | 314.95 | -21.57 | 143.32 | 0.5772 | 642.0 | 526.4 | |
| 0.00 | 6.83 | 0.00 | 4.11 | -18.93 | 313.34 | -23.18 | 139.08 | 0.5707 | 859.0 | 624.5 | |
| 0.00 | 0.80 | 0.00 | 0.48 | -18.77 | 313.12 | -23.40 | 138.63 | 0.5711 | 620.0 | 540.2 | |
| 0.89 | 2.22 | 0.54 | 1.36 | -20.11 | 312.63 | -23.89 | 139.64 | 0.5894 | 737.6 | 590.5 | |
| 0.89 | 1.86 | 0.56 | 1.18 | -21.70 | 310.28 | -26.24 | 138.85 | 0.6266 | -846.3 | -771.6 | |
| 0.00 | 1.24 | 0.00 | 0.79 | -21.30 | 310.10 | -26.42 | 138.21 | 0.6243 | -757.0 | -574.1 | |
| 0.89 | 2.93 | 0.56 | 1.85 | -21.06 | 310.04 | -26.48 | 137.88 | 0.6226 | -872.3 | -675.1 | |
| 0.00 | 2.75 | 0.00 | 1.75 | -21.86 | 309.81 | -26.71 | 138.54 | 0.6324 | -668.0 | -460.0 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -21.17 | 309.95 | -26.57 | 137.90 | 0.6245 | -557.0 | -583.2 | |
| 2.57 | 7.89 | 1.64 | 5.05 | -21.68 | 309.48 | -27.04 | 137.99 | 0.6335 | -862.6 | -531.9 | |
| 0.00 | 1.15 | 0.00 | 0.74 | -22.06 | 309.40 | -27.12 | 138.34 | 0.6378 | -556.0 | -446.0 | |
| 1.33 | -10.00 | 0.85 | -10.00 | -21.59 | 309.25 | -27.27 | 137.65 | 0.6348 | -661.9 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.45 | -20.81 | 308.57 | -27.95 | 136.07 | 0.6339 | -553.0 | -480.9 | |
| 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. | |