SDO HMI 2014-04-09 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.30 | 300.85 | 65.89 | 327.17 | 12.38 | 272.90 | -60.54 | 72.77 | 0.8908 | -255.8 | -83.5 | |
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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 |
| 5.55 | 24.25 | 7.37 | 32.14 | 15.22 | 268.12 | -65.32 | 70.91 | 0.9294 | 479.5 | 188.3 | |
| 1.85 | -1.00 | 2.45 | -1.00 | 14.81 | 268.12 | -65.31 | 71.34 | 0.9288 | 314.3 | 999999 | |
| 1.23 | 59.78 | 1.57 | 76.05 | 14.40 | 268.91 | -64.53 | 71.59 | 0.9232 | 454.2 | 143.3 | |
| 7.14 | -3.00 | 9.06 | -3.00 | 13.89 | 268.94 | -64.50 | 72.12 | 0.9223 | 507.6 | 999999 | |
| 1.59 | -3.00 | 2.01 | -3.00 | 14.20 | 269.08 | -64.36 | 71.76 | 0.9219 | 652.0 | 999999 | |
| 0.00 | 1.76 | 0.00 | 2.15 | 14.13 | 270.07 | -63.37 | 71.59 | 0.9153 | 580.0 | 500.0 | |
| 0.00 | 1.06 | 0.00 | 1.19 | 12.17 | 271.92 | -61.52 | 73.25 | 0.8991 | -5.0 | -21.5 | |
| 0.00 | 0.62 | 0.00 | 0.67 | 11.98 | 272.81 | -60.63 | 73.23 | 0.8922 | -261.0 | -214.3 | |
| 2.56 | 212.59 | 2.70 | 214.13 | 11.86 | 273.70 | -59.74 | 73.14 | 0.8852 | -201.1 | -212.2 | |
| 0.00 | 0.79 | 0.00 | 0.84 | 11.22 | 273.52 | -59.92 | 73.89 | 0.8854 | 303.0 | 251.4 | |
| 40.38 | -9.00 | 40.73 | -9.00 | 11.35 | 275.14 | -58.30 | 73.32 | 0.8728 | -709.1 | 999999 | |
| 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. | |