SDO HMI 2014-11-07 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.93 | 18.14 | 1.87 | 11.16 | -15.64 | 19.05 | -31.07 | 123.18 | 0.5934 | -45.8 | -125.9 | |
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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 | 0.52 | 0.00 | 0.29 | -12.36 | 27.42 | -22.70 | 125.80 | 0.4668 | 777.0 | 647.8 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -12.27 | 27.27 | -22.86 | 125.46 | 0.4680 | 577.0 | 518.7 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -14.49 | 25.53 | -24.60 | 127.27 | 0.5085 | 897.0 | 662.0 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -13.98 | 24.84 | -25.28 | 125.70 | 0.5124 | 778.0 | 647.1 | |
| 0.00 | 1.73 | 0.00 | 1.01 | -14.13 | 22.81 | -27.32 | 123.93 | 0.5385 | 347.0 | 308.5 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -14.32 | 22.78 | -27.34 | 124.20 | 0.5403 | 711.0 | 524.4 | |
| 0.00 | 1.90 | 0.00 | 1.19 | -17.27 | 18.02 | -32.10 | 124.49 | 0.6180 | -694.0 | -530.3 | |
| 0.00 | 0.69 | 0.00 | 0.43 | -15.44 | 17.23 | -32.90 | 121.28 | 0.6148 | 425.0 | 293.4 | |
| 0.00 | 1.12 | 0.00 | 0.71 | -16.48 | 16.40 | -33.72 | 122.15 | 0.6311 | -816.0 | -630.8 | |
| 0.00 | 1.73 | 0.00 | 1.10 | -16.55 | 16.20 | -33.92 | 122.11 | 0.6339 | -823.0 | -709.2 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -17.16 | 15.92 | -34.20 | 122.76 | 0.6410 | -534.0 | -480.8 | |
| 2.93 | 4.49 | 1.87 | 2.87 | -16.17 | 16.01 | -34.11 | 121.45 | 0.6337 | -882.2 | -688.2 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -16.76 | 15.59 | -34.53 | 121.97 | 0.6422 | -630.0 | -458.0 | |
| 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. | |