SDO HMI 2014-08-13 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.55 | 32.82 | 10.34 | 29.20 | -18.35 | 161.21 | 51.00 | 242.65 | 0.8323 | 325.2 | 269.5 | |
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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 | 1.26 | 0.00 | 1.32 | -20.18 | 166.80 | 56.58 | 242.86 | 0.8823 | 305.0 | 226.3 | |
| 4.15 | 11.10 | 3.75 | 10.01 | -16.25 | 162.75 | 52.54 | 245.66 | 0.8384 | 537.2 | 354.0 | |
| 3.70 | -2.00 | 3.33 | -2.00 | -16.36 | 162.53 | 52.32 | 245.46 | 0.8369 | 637.8 | 999999 | |
| 0.00 | 1.26 | 0.00 | 1.16 | -18.49 | 162.40 | 52.19 | 243.03 | 0.8428 | 431.0 | 335.0 | |
| 0.00 | 0.81 | 0.00 | 0.72 | -18.07 | 161.55 | 51.34 | 243.14 | 0.8342 | 435.0 | 396.1 | |
| 3.70 | 9.02 | 3.26 | 7.91 | -19.16 | 160.42 | 50.21 | 241.44 | 0.8285 | 535.2 | 661.5 | |
| 0.00 | 1.44 | 0.00 | 1.25 | -18.79 | 160.02 | 49.80 | 241.68 | 0.8236 | 663.0 | 558.0 | |
| 0.00 | 2.80 | 0.00 | 2.46 | -19.57 | 160.19 | 49.98 | 240.88 | 0.8280 | 605.0 | 487.2 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -19.46 | 159.99 | 49.78 | 240.92 | 0.8259 | 482.0 | 550.7 | |
| 0.00 | 0.45 | 0.00 | 0.38 | -18.49 | 158.57 | 48.36 | 241.36 | 0.8097 | -468.0 | -463.6 | |
| 0.00 | 1.98 | 0.00 | 1.70 | -20.33 | 158.57 | 48.36 | 239.29 | 0.8172 | -613.0 | -491.2 | |
| 0.00 | 1.80 | 0.00 | 1.53 | -20.46 | 158.14 | 47.92 | 238.94 | 0.8140 | -628.0 | -523.5 | |
| 0.00 | 0.63 | 0.00 | 0.52 | -20.85 | 156.05 | 45.84 | 237.46 | 0.7975 | -480.0 | -435.9 | |
| 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. | |