SDO HMI 2014-09-26 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.43 | 159.52 | 64.42 | 223.74 | 12.33 | 168.88 | -70.29 | 79.37 | 0.9356 | -45.8 | 0.7 | |
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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 | 0.71 | 0.00 | 0.85 | 12.09 | 172.50 | -66.67 | 79.82 | 0.9140 | -374.0 | -366.8 | |
| 1.41 | 16.60 | 1.72 | 20.17 | 12.37 | 172.28 | -66.89 | 79.50 | 0.9154 | -701.2 | -438.9 | |
| 0.00 | 0.79 | 0.00 | 0.99 | 12.44 | 171.76 | -67.41 | 79.40 | 0.9189 | -227.0 | -191.9 | |
| 17.04 | 60.12 | 21.31 | 75.75 | 11.82 | 171.68 | -67.49 | 80.08 | 0.9196 | -624.9 | -208.3 | |
| 3.35 | -4.00 | 4.32 | -4.00 | 11.95 | 170.95 | -68.22 | 79.90 | 0.9244 | -72.4 | 999999 | |
| 0.00 | 0.97 | 0.00 | 1.22 | 10.38 | 171.71 | -67.46 | 81.64 | 0.9199 | -370.0 | -370.6 | |
| 0.00 | 1.85 | 0.00 | 2.46 | 12.21 | 170.21 | -68.96 | 79.59 | 0.9291 | 398.0 | 324.1 | |
| 0.00 | 0.97 | 0.00 | 1.27 | 11.77 | 170.45 | -68.72 | 80.07 | 0.9277 | 403.0 | 363.3 | |
| 0.00 | 2.21 | 0.00 | 2.98 | 12.22 | 169.77 | -69.40 | 79.55 | 0.9319 | -15.0 | 83.6 | |
| 7.06 | 44.40 | 10.13 | 62.86 | 12.86 | 168.36 | -70.81 | 78.79 | 0.9401 | 668.6 | 264.3 | |
| 0.00 | 1.41 | 0.00 | 2.10 | 12.93 | 167.63 | -71.53 | 78.68 | 0.9442 | 335.0 | 269.4 | |
| 7.42 | 15.27 | 11.18 | 23.10 | 12.62 | 167.35 | -71.82 | 78.99 | 0.9459 | 392.0 | 155.0 | |
| 0.00 | 1.59 | 0.00 | 2.51 | 11.39 | 166.53 | -72.63 | 80.24 | 0.9507 | 380.0 | 307.5 | |
| 1.50 | 3.71 | 2.96 | 7.30 | 12.92 | 162.62 | -76.54 | 78.40 | 0.9688 | -136.7 | -10.9 | |
| 5.65 | 8.92 | 12.80 | 20.18 | 12.19 | 160.59 | -78.57 | 79.00 | 0.9770 | 18.5 | 138.1 | |
| 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. | |