SDO HMI 2014-09-05 00:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.32 | 0.00 | 9.38 | 9.87 | 181.07 | 13.11 | 278.87 | 0.2401 | -190.7 | -256.5 | |
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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 | 1.70 | 0.00 | 0.89 | 11.37 | 187.79 | 19.83 | 283.39 | 0.3434 | -898.0 | -692.6 | |
| 0.00 | 1.25 | 0.00 | 0.66 | 10.84 | 187.36 | 19.40 | 282.05 | 0.3351 | -910.0 | -756.9 | |
| 0.00 | 1.79 | 0.00 | 0.93 | 11.17 | 186.57 | 18.61 | 283.46 | 0.3234 | -888.0 | -631.2 | |
| 0.00 | 3.04 | 0.00 | 1.58 | 10.74 | 185.96 | 18.00 | 282.45 | 0.3123 | -658.0 | -613.9 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 11.30 | 185.74 | 17.78 | 284.34 | 0.3104 | -808.0 | -640.3 | |
| 0.00 | 2.05 | 0.00 | 1.07 | 10.88 | 185.64 | 17.69 | 283.05 | 0.3076 | -822.0 | -672.3 | |
| 0.00 | 1.52 | 0.00 | 0.75 | 9.55 | 171.75 | 3.79 | 301.83 | 0.0770 | 903.0 | 752.8 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 11.70 | 171.53 | 3.57 | 321.94 | 0.0994 | 878.0 | 737.7 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 11.61 | 171.44 | 3.48 | 322.10 | 0.0971 | 808.0 | 599.1 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 2.94 | 170.87 | 2.91 | 214.09 | 0.0910 | -705.0 | -555.3 | |
| 0.00 | 1.52 | 0.00 | 0.75 | 2.79 | 169.39 | 1.43 | 197.81 | 0.0819 | 1002.0 | 754.1 | |
| 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. | |