SDO HMI 2014-07-02 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.15 | 127.43 | 52.95 | 171.20 | -8.11 | 238.85 | -67.54 | 99.94 | 0.9299 | 149.9 | -156.3 | |
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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 |
| 2.27 | 3.91 | 2.74 | 4.71 | -8.13 | 241.42 | -64.97 | 100.30 | 0.9133 | 461.4 | 432.6 | |
| 0.91 | 3.18 | 1.12 | 3.91 | -8.62 | 240.97 | -65.42 | 100.77 | 0.9169 | 558.0 | 433.8 | |
| 0.00 | 1.63 | 0.00 | 2.02 | -8.10 | 240.84 | -65.55 | 100.19 | 0.9174 | 442.0 | 408.8 | |
| 10.99 | 44.42 | 13.51 | 55.89 | -7.39 | 240.83 | -65.56 | 99.41 | 0.9168 | 693.5 | -121.8 | |
| 7.63 | -4.00 | 9.61 | -4.00 | -7.42 | 240.21 | -66.18 | 99.37 | 0.9210 | 328.7 | 999999 | |
| 3.45 | 15.44 | 4.50 | 20.22 | -8.84 | 239.58 | -66.81 | 100.82 | 0.9263 | 300.9 | -32.3 | |
| 0.82 | 13.90 | 1.06 | 18.43 | -7.36 | 239.45 | -66.94 | 99.22 | 0.9261 | 308.8 | -3.8 | |
| 2.91 | -7.00 | 3.83 | -7.00 | -7.22 | 239.09 | -67.30 | 99.03 | 0.9283 | 315.3 | 999999 | |
| 1.63 | 7.81 | 2.22 | 10.60 | -8.49 | 238.58 | -67.81 | 100.32 | 0.9324 | -485.4 | -485.2 | |
| 0.00 | 2.72 | 0.00 | 3.65 | -7.55 | 238.74 | -67.65 | 99.34 | 0.9307 | -454.0 | -397.6 | |
| 0.00 | 1.54 | 0.00 | 2.21 | -9.84 | 237.50 | -68.88 | 101.63 | 0.9399 | -197.0 | -205.4 | |
| 0.00 | 0.73 | 0.00 | 1.06 | -9.49 | 237.14 | -69.25 | 101.21 | 0.9417 | -494.0 | -458.4 | |
| 0.00 | 5.45 | 0.00 | 8.30 | -9.04 | 236.17 | -70.22 | 100.62 | 0.9469 | 80.0 | 90.7 | |
| 9.54 | 25.43 | 14.36 | 37.83 | -8.54 | 236.30 | -70.09 | 100.10 | 0.9459 | -414.7 | -441.4 | |
| 0.00 | 0.27 | 0.00 | 0.50 | -10.94 | 233.12 | -73.26 | 102.25 | 0.9633 | -325.0 | -344.3 | |
| 0.00 | 1.00 | 0.00 | 1.87 | -10.93 | 232.69 | -73.70 | 102.19 | 0.9653 | -338.0 | -313.5 | |
| 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. | |