SDO HMI 2014-09-06 19:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.96 | 48.62 | 17.61 | 70.73 | -20.56 | 78.76 | -65.55 | 115.01 | 0.9411 | -45.6 | -136.9 | |
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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 | 2.14 | 0.00 | 2.70 | -20.66 | 82.38 | -61.93 | 116.16 | 0.9215 | 474.0 | 401.4 | |
| 1.52 | 5.71 | 1.96 | 7.41 | -20.44 | 81.70 | -62.61 | 115.72 | 0.9251 | 343.2 | 296.2 | |
| 0.00 | 0.89 | 0.00 | 1.18 | -20.55 | 81.05 | -63.26 | 115.64 | 0.9292 | -295.0 | -270.3 | |
| 0.00 | 1.34 | 0.00 | 1.77 | -20.38 | 81.10 | -63.20 | 115.48 | 0.9285 | -179.0 | -131.3 | |
| 1.52 | 4.28 | 2.12 | 6.02 | -21.64 | 80.03 | -64.27 | 116.46 | 0.9369 | 483.5 | 243.9 | |
| 0.45 | 1.61 | 0.54 | 1.95 | -17.68 | 82.50 | -61.80 | 113.09 | 0.9146 | 452.8 | 327.5 | |
| 2.94 | 5.00 | 4.13 | 7.01 | -21.29 | 79.87 | -64.44 | 116.05 | 0.9371 | 62.0 | 18.5 | |
| 0.00 | 0.98 | 0.00 | 1.40 | -20.14 | 79.20 | -65.11 | 114.68 | 0.9388 | -417.0 | -426.5 | |
| 0.00 | 1.96 | 0.00 | 2.78 | -19.90 | 79.23 | -65.07 | 114.45 | 0.9382 | -563.0 | -487.4 | |
| 4.19 | 20.43 | 6.23 | 30.09 | -20.03 | 78.19 | -66.12 | 114.29 | 0.9440 | -374.2 | -371.0 | |
| 1.34 | 4.28 | 2.63 | 8.42 | -22.16 | 73.28 | -71.03 | 115.20 | 0.9691 | 31.6 | -13.6 | |
| 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. | |