SDO HMI 2014-07-02 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.70 | 120.32 | 44.04 | 164.70 | -8.07 | 238.92 | -68.02 | 99.85 | 0.9329 | 175.4 | -104.4 | |
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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 |
| 2.63 | 4.36 | 3.24 | 5.37 | -8.13 | 241.39 | -65.55 | 100.22 | 0.9174 | 511.0 | 414.4 | |
| 0.00 | 1.54 | 0.00 | 1.89 | -7.48 | 241.44 | -65.50 | 99.52 | 0.9165 | 151.0 | 138.6 | |
| 2.27 | 3.91 | 2.86 | 4.91 | -8.62 | 240.92 | -66.02 | 100.69 | 0.9209 | 429.1 | 331.2 | |
| 0.00 | 1.63 | 0.00 | 2.06 | -8.07 | 240.80 | -66.14 | 100.07 | 0.9213 | 416.0 | 371.5 | |
| 8.81 | 39.14 | 11.10 | 50.38 | -7.39 | 240.78 | -66.16 | 99.34 | 0.9209 | 688.8 | -54.7 | |
| 7.36 | -5.00 | 9.51 | -5.00 | -7.42 | 240.15 | -66.79 | 99.29 | 0.9251 | 283.6 | 999999 | |
| 3.00 | 16.89 | 4.00 | 22.69 | -8.88 | 239.48 | -67.45 | 100.78 | 0.9305 | 311.9 | -9.0 | |
| 0.00 | 7.72 | 0.00 | 10.72 | -8.61 | 238.59 | -68.35 | 100.38 | 0.9358 | -455.0 | -438.4 | |
| 0.00 | 15.89 | 0.00 | 21.68 | -7.29 | 238.89 | -68.04 | 99.01 | 0.9330 | 218.0 | 9.4 | |
| 0.00 | 0.27 | 0.00 | 0.41 | -9.52 | 237.15 | -69.79 | 101.17 | 0.9448 | -457.0 | -464.0 | |
| 8.63 | 24.79 | 13.33 | 37.94 | -8.50 | 236.32 | -70.62 | 100.01 | 0.9488 | -393.9 | -393.1 | |
| 0.00 | 3.91 | 0.00 | 6.14 | -9.04 | 236.07 | -70.87 | 100.55 | 0.9504 | 217.0 | 183.7 | |
| 0.00 | 0.27 | 0.00 | 0.51 | -10.97 | 233.11 | -73.83 | 102.22 | 0.9659 | -361.0 | -316.7 | |
| 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. | |