SDO HMI 2011-07-05 01:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.96 | 266.81 | 24.26 | 146.37 | 16.80 | 354.43 | 21.85 | 303.94 | 0.4307 | -428.3 | -253.3 | |
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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 | 1.09 | 0.00 | 0.60 | 15.45 | 356.46 | 23.88 | 298.92 | 0.4476 | 607.0 | 530.4 | |
| 34.88 | 218.55 | 19.27 | 120.60 | 16.72 | 355.51 | 22.93 | 302.41 | 0.4438 | -1164.1 | -377.1 | |
| 9.08 | -2.00 | 4.99 | -2.00 | 16.86 | 354.80 | 22.22 | 303.44 | 0.4355 | -1190.0 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 14.66 | 353.97 | 21.39 | 299.69 | 0.4079 | -759.0 | -556.9 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 19.68 | 354.21 | 21.63 | 309.52 | 0.4518 | -701.0 | -605.9 | |
| 0.00 | 1.73 | 0.00 | 0.94 | 16.94 | 353.82 | 21.24 | 304.71 | 0.4233 | -917.0 | -747.6 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 19.67 | 353.55 | 20.97 | 310.30 | 0.4437 | -676.0 | -547.8 | |
| 0.00 | 1.64 | 0.00 | 0.88 | 15.87 | 352.54 | 19.96 | 303.99 | 0.3978 | -870.0 | -735.1 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 16.25 | 352.28 | 19.70 | 305.14 | 0.3974 | -597.0 | -514.2 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 15.32 | 351.78 | 19.20 | 303.73 | 0.3831 | -797.0 | -602.5 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 19.25 | 352.05 | 19.47 | 311.50 | 0.4218 | -636.0 | -507.6 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 20.24 | 352.10 | 19.52 | 313.24 | 0.4322 | -706.0 | -616.9 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 19.10 | 351.58 | 19.00 | 311.86 | 0.4149 | -752.0 | -583.5 | |
| 0.00 | 1.73 | 0.00 | 0.94 | 20.09 | 351.19 | 18.61 | 314.27 | 0.4203 | -813.0 | -648.6 | |
| 0.00 | 2.91 | 0.00 | 1.55 | 16.00 | 350.45 | 17.87 | 307.10 | 0.3713 | 803.0 | 686.8 | |
| 0.00 | 0.64 | 0.00 | 0.33 | 12.68 | 349.98 | 17.40 | 299.66 | 0.3371 | 762.0 | 611.1 | |
| 0.00 | 3.82 | 0.00 | 2.03 | 16.16 | 350.16 | 17.58 | 307.88 | 0.3691 | 660.0 | 679.8 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 12.78 | 349.72 | 17.14 | 300.26 | 0.3342 | 1009.0 | 767.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 19.66 | 350.22 | 17.64 | 314.94 | 0.4048 | -797.0 | -658.7 | |
| 0.00 | 2.91 | 0.00 | 1.55 | 16.70 | 349.74 | 17.16 | 309.71 | 0.3690 | 627.0 | 511.7 | |
| 0.00 | 1.73 | 0.00 | 0.93 | 19.07 | 349.81 | 17.23 | 314.44 | 0.3939 | -815.0 | -579.2 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 16.55 | 349.43 | 16.85 | 309.87 | 0.3636 | 750.0 | 666.5 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 16.99 | 349.31 | 16.72 | 311.03 | 0.3664 | 869.0 | 791.2 | |
| 0.00 | 2.00 | 0.00 | 1.06 | 16.68 | 349.24 | 16.66 | 310.45 | 0.3625 | 1039.0 | 907.4 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 16.66 | 348.41 | 15.83 | 311.79 | 0.3521 | 833.0 | 635.8 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 17.02 | 347.75 | 15.17 | 313.75 | 0.3478 | 883.0 | 654.7 | |
| 0.00 | 2.18 | 0.00 | 1.15 | 17.61 | 347.73 | 15.15 | 315.05 | 0.3542 | 785.0 | 745.8 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 18.22 | 347.35 | 14.77 | 316.99 | 0.3567 | 674.0 | 515.0 | |
| 0.00 | 1.91 | 0.00 | 1.01 | 17.56 | 347.10 | 14.52 | 316.12 | 0.3463 | 818.0 | 657.2 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 18.35 | 346.93 | 14.35 | 318.05 | 0.3535 | 801.0 | 614.3 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 16.13 | 345.94 | 13.36 | 315.26 | 0.3168 | 894.0 | 694.3 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 16.66 | 345.98 | 13.40 | 316.40 | 0.3233 | 819.0 | 669.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 16.88 | 345.96 | 13.38 | 316.92 | 0.3256 | 905.0 | 605.7 | |
| 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. | |