SDO HMI 2014-10-13 04:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.43 | 291.39 | 55.83 | 375.73 | -8.90 | 318.43 | -65.77 | 102.35 | 0.9211 | 566.5 | 181.6 | |
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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 | 1.23 | 0.00 | 1.46 | -10.57 | 320.60 | -63.60 | 104.54 | 0.9114 | 245.0 | 170.5 | |
| 29.76 | 241.84 | 34.70 | 281.73 | -9.03 | 320.87 | -63.33 | 102.93 | 0.9073 | 730.4 | 191.7 | |
| 11.55 | -2.00 | 13.37 | -2.00 | -8.49 | 321.04 | -63.16 | 102.38 | 0.9053 | 781.6 | 999999 | |
| 0.00 | 1.58 | 0.00 | 2.00 | -9.75 | 318.85 | -65.35 | 103.29 | 0.9221 | 248.0 | 187.1 | |
| 0.00 | 1.58 | 0.00 | 1.99 | -9.26 | 318.81 | -65.39 | 102.76 | 0.9217 | 256.0 | 204.2 | |
| 0.00 | 0.35 | 0.00 | 0.44 | -9.04 | 318.60 | -65.60 | 102.48 | 0.9228 | 11.0 | 76.8 | |
| 0.00 | 0.79 | 0.00 | 1.00 | -8.78 | 318.69 | -65.51 | 102.22 | 0.9219 | 205.0 | 173.7 | |
| 0.88 | 3.41 | 1.36 | 5.31 | -8.56 | 314.06 | -70.14 | 101.15 | 0.9493 | -480.0 | -412.3 | |
| 0.00 | 1.75 | 0.00 | 2.94 | -9.34 | 312.76 | -71.43 | 101.74 | 0.9567 | -292.0 | -257.4 | |
| 0.88 | 38.86 | 1.73 | 78.86 | -9.07 | 309.99 | -74.21 | 101.01 | 0.9692 | -144.0 | 199.7 | |
| 2.36 | -10.00 | 4.67 | -10.00 | -8.88 | 309.98 | -74.22 | 100.82 | 0.9691 | -115.6 | 999999 | |
| 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. | |