SDO HMI 2014-09-20 10:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.89 | 13.74 | 0.52 | 8.00 | -21.26 | 310.22 | -14.20 | 154.19 | 0.5261 | -393.3 | -416.4 | |
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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 | 0.44 | 0.00 | 0.25 | -19.07 | 314.04 | -10.38 | 158.81 | 0.4728 | 557.0 | 498.4 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -18.87 | 313.83 | -10.59 | 158.25 | 0.4712 | 803.0 | 670.9 | |
| 0.00 | 0.80 | 0.00 | 0.47 | -22.19 | 311.73 | -12.69 | 157.30 | 0.5293 | -610.0 | -482.8 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -21.86 | 310.29 | -14.13 | 154.76 | 0.5334 | -596.0 | -485.5 | |
| 0.00 | 1.06 | 0.00 | 0.62 | -22.00 | 310.07 | -14.34 | 154.55 | 0.5367 | -631.0 | -506.9 | |
| 0.00 | 1.42 | 0.00 | 0.83 | -21.55 | 310.09 | -14.33 | 154.18 | 0.5307 | -825.0 | -607.2 | |
| 0.00 | 1.24 | 0.00 | 0.72 | -20.97 | 310.11 | -14.31 | 153.70 | 0.5229 | -432.0 | -476.8 | |
| 0.00 | 1.06 | 0.00 | 0.62 | -22.11 | 309.93 | -14.49 | 154.42 | 0.5390 | -572.0 | -527.2 | |
| 0.00 | 0.35 | 0.00 | 0.21 | -21.35 | 309.87 | -14.55 | 153.67 | 0.5295 | -485.0 | -609.2 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -21.87 | 309.68 | -14.73 | 153.84 | 0.5375 | -790.0 | -720.8 | |
| 0.89 | 1.86 | 0.52 | 1.09 | -21.68 | 309.44 | -14.98 | 153.29 | 0.5366 | -864.5 | -637.6 | |
| 0.00 | 1.51 | 0.00 | 0.88 | -20.81 | 308.83 | -15.59 | 151.55 | 0.5295 | -620.0 | -629.2 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -20.78 | 308.56 | -15.86 | 151.12 | 0.5311 | -274.0 | -331.8 | |
| 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. | |