SDO HMI 2014-09-29 22:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.58 | 0.00 | 9.67 | -22.80 | 195.60 | -3.42 | 175.12 | 0.5140 | -255.7 | -220.5 | |
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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 | 0.97 | 0.00 | 0.54 | -18.62 | 210.18 | 11.15 | 203.24 | 0.4666 | 704.0 | 567.1 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -21.45 | 210.22 | 11.19 | 200.98 | 0.5065 | 569.0 | 382.2 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -26.69 | 210.07 | 11.05 | 197.30 | 0.5780 | 539.0 | 478.9 | |
| 0.00 | 1.50 | 0.00 | 0.87 | -24.46 | 205.13 | 6.10 | 190.58 | 0.5292 | 577.0 | 477.7 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -13.28 | 202.61 | 3.58 | 190.05 | 0.3498 | -11.0 | -11.3 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -16.53 | 201.18 | 2.16 | 185.21 | 0.3992 | -808.0 | -559.2 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -13.46 | 201.06 | 2.04 | 185.71 | 0.3493 | -21.0 | -17.2 | |
| 0.00 | 1.59 | 0.00 | 0.88 | -20.51 | 198.34 | -0.68 | 178.61 | 0.4607 | -786.0 | -630.0 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -7.01 | 192.97 | -6.05 | 156.26 | 0.2610 | -871.0 | -727.8 | |
| 0.00 | 0.97 | 0.00 | 0.63 | -33.13 | 191.08 | -7.94 | 169.77 | 0.6535 | -316.0 | -255.6 | |
| 0.00 | 1.23 | 0.00 | 0.79 | -31.97 | 190.87 | -8.16 | 169.10 | 0.6388 | -699.0 | -545.4 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -13.38 | 191.35 | -7.67 | 159.30 | 0.3690 | -760.0 | -547.5 | |
| 0.00 | 1.15 | 0.00 | 0.75 | -32.73 | 187.75 | -11.27 | 165.47 | 0.6577 | -640.0 | -526.3 | |
| 0.00 | 1.59 | 0.00 | 1.00 | -27.21 | 180.87 | -18.15 | 153.43 | 0.6217 | -644.0 | -408.2 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -27.50 | 177.55 | -21.48 | 149.71 | 0.6463 | -668.0 | -465.6 | |
| 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. | |