SDO HMI 2014-09-07 04:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.85 | 60.24 | 10.23 | 32.72 | -14.67 | 149.45 | 10.10 | 204.66 | 0.4104 | -115.1 | 82.8 | |
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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 | 2.05 | 0.00 | 1.13 | -15.97 | 150.15 | 10.80 | 204.68 | 0.4334 | -900.0 | -702.3 | |
| 0.00 | 2.14 | 0.00 | 1.18 | -16.66 | 150.19 | 10.84 | 204.07 | 0.4435 | -726.0 | -411.5 | |
| 5.45 | 21.96 | 2.92 | 11.80 | -12.90 | 149.87 | 10.53 | 207.47 | 0.3877 | 1120.1 | 800.0 | |
| 1.79 | -3.00 | 0.96 | -3.00 | -13.13 | 149.79 | 10.44 | 207.01 | 0.3903 | 1044.3 | 999999 | |
| 0.00 | 2.23 | 0.00 | 1.20 | -13.61 | 149.62 | 10.27 | 206.08 | 0.3960 | 540.0 | 441.3 | |
| 2.41 | 5.98 | 1.29 | 3.20 | -12.67 | 149.55 | 10.20 | 207.02 | 0.3820 | 1063.6 | 728.8 | |
| 3.04 | 19.73 | 1.67 | 10.86 | -16.55 | 149.60 | 10.26 | 203.02 | 0.4382 | -909.4 | -772.7 | |
| 0.00 | 1.52 | 0.00 | 0.84 | -17.47 | 149.52 | 10.18 | 202.03 | 0.4511 | -668.0 | -390.9 | |
| 4.55 | -7.00 | 2.51 | -7.00 | -16.61 | 149.35 | 10.00 | 202.46 | 0.4375 | -1065.5 | 999999 | |
| 1.61 | -7.00 | 0.88 | -7.00 | -16.57 | 149.19 | 9.84 | 202.16 | 0.4361 | -1070.3 | 999999 | |
| 0.00 | 1.87 | 0.00 | 1.01 | -13.95 | 147.71 | 8.36 | 201.39 | 0.3887 | 838.0 | 606.8 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -16.07 | 147.60 | 8.25 | 199.27 | 0.4199 | -728.0 | -530.3 | |
| 0.00 | 1.96 | 0.00 | 1.06 | -15.67 | 145.66 | 6.31 | 195.22 | 0.4047 | -849.0 | -646.3 | |
| 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. | |