SDO HMI 2014-09-07 13:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.25 | 76.74 | 17.86 | 132.47 | -16.51 | 64.36 | -70.06 | 109.74 | 0.9581 | 235.2 | -44.8 | |
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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 | 0.45 | 0.00 | 0.69 | -16.97 | 66.50 | -67.91 | 110.70 | 0.9488 | 464.0 | 408.8 | |
| 4.02 | 54.25 | 6.33 | 86.84 | -16.89 | 66.05 | -68.37 | 110.51 | 0.9510 | 444.5 | 60.0 | |
| 4.91 | -2.00 | 7.79 | -2.00 | -16.46 | 65.86 | -68.56 | 110.02 | 0.9514 | 535.5 | 999999 | |
| 2.32 | -2.00 | 3.74 | -2.00 | -16.69 | 65.59 | -68.82 | 110.19 | 0.9530 | 118.5 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.90 | -16.69 | 64.78 | -69.63 | 110.00 | 0.9569 | -121.0 | -124.5 | |
| 0.00 | 2.50 | 0.00 | 4.38 | -16.99 | 64.15 | -70.26 | 110.17 | 0.9602 | 77.0 | 23.4 | |
| 0.00 | 0.62 | 0.00 | 1.15 | -16.85 | 63.21 | -71.20 | 109.81 | 0.9642 | -25.0 | -100.6 | |
| 0.00 | 0.71 | 0.00 | 1.26 | -16.11 | 63.76 | -70.65 | 109.18 | 0.9610 | 44.0 | 76.2 | |
| 0.00 | 1.16 | 0.00 | 2.14 | -16.64 | 63.10 | -71.31 | 109.57 | 0.9644 | -60.0 | -27.6 | |
| 0.00 | 1.78 | 0.00 | 3.78 | -16.43 | 60.86 | -73.55 | 108.89 | 0.9733 | -443.0 | -424.5 | |
| 0.00 | 0.27 | 0.00 | 0.58 | -16.69 | 60.59 | -73.82 | 109.10 | 0.9745 | -297.0 | -310.0 | |
| 0.00 | 8.66 | 0.00 | 17.93 | -16.08 | 61.10 | -73.31 | 108.59 | 0.9721 | -530.0 | -461.5 | |
| 0.00 | 5.80 | 0.00 | 12.82 | -15.87 | 60.16 | -74.25 | 108.19 | 0.9755 | 14.0 | 46.3 | |
| 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. | |