SDO HMI 2014-08-07 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.10 | 48.18 | 19.10 | 61.12 | -20.44 | 251.53 | 62.53 | 244.64 | 0.9214 | 197.0 | 5.7 | |
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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 | 4.52 | 0.00 | 5.98 | -19.87 | 252.92 | 63.92 | 245.64 | 0.9289 | -171.0 | -153.5 | |
| 3.44 | 26.76 | 4.45 | 35.17 | -19.91 | 252.36 | 63.37 | 245.44 | 0.9257 | 515.0 | 40.7 | |
| 2.26 | -2.00 | 2.96 | -2.00 | -20.20 | 252.58 | 63.58 | 245.20 | 0.9275 | 430.9 | 999999 | |
| 1.63 | -2.00 | 2.14 | -2.00 | -20.47 | 252.55 | 63.56 | 244.92 | 0.9278 | 472.9 | 999999 | |
| 0.00 | 0.90 | 0.00 | 1.15 | -19.64 | 251.95 | 62.95 | 245.61 | 0.9227 | 416.0 | 383.7 | |
| 3.34 | -2.00 | 4.40 | -2.00 | -20.63 | 252.53 | 63.53 | 244.74 | 0.9280 | 341.8 | 999999 | |
| 0.00 | 1.27 | 0.00 | 1.63 | -20.19 | 252.13 | 63.13 | 245.08 | 0.9248 | 526.0 | 510.9 | |
| 0.00 | 0.90 | 0.00 | 1.07 | -19.80 | 249.91 | 60.91 | 244.84 | 0.9101 | 123.0 | 233.9 | |
| 2.17 | 7.96 | 2.54 | 9.34 | -20.87 | 249.22 | 60.22 | 243.51 | 0.9079 | -140.7 | 4.0 | |
| 0.72 | 1.99 | 0.84 | 2.31 | -21.16 | 248.82 | 59.83 | 243.07 | 0.9060 | -336.0 | -204.9 | |
| 1.54 | 2.62 | 1.77 | 3.02 | -21.34 | 248.55 | 59.55 | 242.80 | 0.9046 | -479.8 | -449.0 | |
| 0.00 | 0.72 | 0.00 | 0.83 | -21.95 | 248.25 | 59.25 | 242.06 | 0.9041 | -588.0 | -522.0 | |
| 0.00 | 0.54 | 0.00 | 0.62 | -22.08 | 247.82 | 58.82 | 241.78 | 0.9016 | 43.0 | 62.8 | |
| 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. | |