SDO HMI 2014-08-07 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.71 | 20.80 | 1.70 | 13.09 | -20.28 | 158.43 | -27.83 | 134.71 | 0.6191 | 423.1 | 377.6 | |
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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 |
| 0.00 | 1.54 | 0.00 | 0.95 | -20.46 | 160.41 | -25.85 | 137.04 | 0.6016 | 771.0 | 479.9 | |
| 0.00 | 1.54 | 0.00 | 0.96 | -20.21 | 159.48 | -26.78 | 135.74 | 0.6081 | 741.0 | 466.5 | |
| 0.00 | 2.35 | 0.00 | 1.48 | -21.10 | 159.27 | -26.99 | 136.60 | 0.6184 | 695.0 | 528.6 | |
| 0.00 | 0.99 | 0.00 | 0.60 | -17.68 | 159.81 | -26.45 | 132.87 | 0.5813 | 609.0 | 433.7 | |
| 2.71 | 4.43 | 1.70 | 2.78 | -20.58 | 158.86 | -27.40 | 135.55 | 0.6175 | 895.8 | 669.3 | |
| 0.00 | 1.72 | 0.00 | 1.08 | -20.59 | 158.60 | -27.66 | 135.30 | 0.6201 | 599.0 | 574.5 | |
| 0.00 | 2.17 | 0.00 | 1.40 | -22.22 | 158.11 | -28.15 | 136.74 | 0.6396 | 367.0 | 326.5 | |
| 0.00 | 1.18 | 0.00 | 0.75 | -21.24 | 157.98 | -28.27 | 135.47 | 0.6318 | 535.0 | 349.1 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -20.49 | 157.88 | -28.38 | 134.47 | 0.6261 | 654.0 | 508.5 | |
| 0.00 | 0.72 | 0.00 | 0.46 | -20.85 | 156.95 | -29.31 | 134.01 | 0.6382 | 355.0 | 301.8 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -12.82 | 157.91 | -28.35 | 124.08 | 0.5611 | 346.0 | 344.5 | |
| 0.00 | 0.72 | 0.00 | 0.48 | -22.02 | 154.35 | -31.90 | 133.06 | 0.6728 | -603.0 | -530.4 | |
| 0.00 | 0.72 | 0.00 | 0.48 | -21.11 | 154.24 | -32.02 | 131.87 | 0.6666 | -795.0 | -636.9 | |
| 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. | |