SDO HMI 2014-09-07 11:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.45 | 140.14 | 35.79 | 145.39 | -9.23 | 194.82 | 59.31 | 255.29 | 0.8787 | 128.5 | -1.6 | |
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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 |
| 20.35 | 77.74 | 22.37 | 85.82 | -9.25 | 196.73 | 61.22 | 255.78 | 0.8943 | 695.6 | 132.2 | |
| 0.00 | 0.27 | 0.00 | 0.27 | -9.07 | 194.33 | 58.82 | 255.36 | 0.8752 | 538.0 | 471.3 | |
| 0.89 | 4.91 | 0.90 | 4.97 | -9.65 | 193.90 | 58.39 | 254.60 | 0.8728 | 633.5 | 444.7 | |
| 0.00 | 6.16 | 0.00 | 5.94 | -8.94 | 192.56 | 57.05 | 255.02 | 0.8601 | -379.0 | -351.4 | |
| 0.00 | 0.98 | 0.00 | 0.95 | -9.44 | 192.63 | 57.12 | 254.47 | 0.8618 | -132.0 | -61.0 | |
| 0.00 | 0.27 | 0.00 | 0.26 | -9.44 | 192.35 | 56.83 | 254.39 | 0.8594 | 225.0 | 188.7 | |
| 0.00 | 1.61 | 0.00 | 1.53 | -8.78 | 192.02 | 56.50 | 255.04 | 0.8551 | -37.0 | -247.1 | |
| 3.66 | 41.68 | 3.48 | 39.54 | -9.06 | 191.97 | 56.46 | 254.72 | 0.8553 | -567.3 | -186.2 | |
| 0.00 | 1.25 | 0.00 | 1.17 | -8.10 | 191.75 | 56.24 | 255.75 | 0.8513 | -241.0 | -288.9 | |
| 0.00 | 2.86 | 0.00 | 2.69 | -8.69 | 191.72 | 56.20 | 255.07 | 0.8523 | -714.0 | -576.3 | |
| 0.00 | 1.61 | 0.00 | 1.50 | -8.29 | 191.52 | 56.01 | 255.46 | 0.8496 | -569.0 | -499.8 | |
| 9.55 | -8.00 | 9.04 | -8.00 | -9.41 | 191.72 | 56.21 | 254.25 | 0.8539 | -719.2 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.75 | -8.59 | 191.36 | 55.85 | 255.08 | 0.8489 | -589.0 | -481.1 | |
| 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. | |