SDO HMI 2014-03-06 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.95 | 123.31 | 28.31 | 134.54 | -9.95 | 359.60 | -63.81 | 97.51 | 0.8932 | 477.2 | 289.2 | |
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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 |
| 1.38 | 104.35 | 1.48 | 112.11 | -10.54 | 0.19 | -63.22 | 98.14 | 0.8886 | 1040.1 | 377.4 | |
| 9.00 | -1.00 | 9.73 | -1.00 | -10.38 | 359.90 | -63.51 | 97.98 | 0.8908 | 670.7 | 999999 | |
| 11.25 | -1.00 | 12.08 | -1.00 | -9.51 | 0.15 | -63.26 | 96.98 | 0.8893 | 730.3 | 999999 | |
| 1.47 | -1.00 | 1.59 | -1.00 | -10.06 | 359.95 | -63.45 | 97.61 | 0.8906 | 633.7 | 999999 | |
| 0.00 | 3.11 | 0.00 | 3.38 | -8.16 | 359.96 | -63.45 | 95.48 | 0.8914 | -558.0 | -413.9 | |
| 0.69 | 1.47 | 0.80 | 1.71 | -10.79 | 357.89 | -65.52 | 98.55 | 0.9058 | 253.0 | 170.8 | |
| 0.00 | 0.52 | 0.00 | 0.66 | -15.38 | 355.11 | -68.30 | 103.69 | 0.9237 | -350.0 | -332.3 | |
| 0.00 | 1.04 | 0.00 | 1.25 | -12.45 | 356.73 | -66.68 | 100.43 | 0.9135 | 437.0 | 352.9 | |
| 0.00 | 1.04 | 0.00 | 1.21 | -9.70 | 357.89 | -65.52 | 97.34 | 0.9063 | 388.0 | 302.7 | |
| 0.00 | 0.87 | 0.00 | 1.02 | -8.88 | 357.60 | -65.81 | 96.46 | 0.9088 | 602.0 | 545.4 | |
| 0.00 | 2.42 | 0.00 | 2.87 | -9.04 | 357.39 | -66.02 | 96.65 | 0.9102 | 161.0 | 132.4 | |
| 1.73 | 6.06 | 2.09 | 7.30 | -10.25 | 356.84 | -66.57 | 98.01 | 0.9135 | -562.9 | -387.1 | |
| 0.00 | 0.78 | 0.00 | 0.93 | -8.76 | 357.34 | -66.07 | 96.35 | 0.9107 | 313.0 | 235.3 | |
| 0.43 | 1.30 | 0.54 | 1.62 | -9.55 | 356.04 | -67.37 | 97.30 | 0.9194 | -442.4 | -442.6 | |
| 0.00 | 0.35 | 0.00 | 0.48 | -14.25 | 353.28 | -70.13 | 102.53 | 0.9353 | -349.0 | -416.5 | |
| 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. | |