SDO HMI 2011-07-01 14:59:11 UT
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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.66 | 285.88 | 43.18 | 163.66 | 16.18 | 351.15 | -27.23 | 61.73 | 0.5006 | -70.6 | 46.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-01 14:59:11 UT
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 | 0.54 | 0.00 | 0.30 | 19.88 | 358.00 | -20.39 | 47.97 | 0.4428 | -543.0 | -674.5 | |
| 0.00 | 0.64 | 0.00 | 0.35 | 18.82 | 357.69 | -20.70 | 50.30 | 0.4366 | -740.0 | -583.3 | |
| 0.00 | 2.09 | 0.00 | 1.16 | 16.46 | 354.47 | -23.92 | 58.43 | 0.4582 | -828.0 | -629.7 | |
| 0.00 | 1.73 | 0.00 | 0.98 | 19.80 | 353.87 | -24.52 | 52.90 | 0.4915 | -775.0 | -571.6 | |
| 0.82 | 126.05 | 0.46 | 70.74 | 15.66 | 353.63 | -24.75 | 60.77 | 0.4638 | -1073.0 | -444.0 | |
| 2.63 | -5.00 | 1.47 | -5.00 | 15.44 | 353.52 | -24.86 | 61.30 | 0.4639 | -972.5 | 999999 | |
| 33.78 | -5.00 | 18.95 | -5.00 | 16.09 | 353.36 | -25.02 | 60.16 | 0.4703 | -1097.7 | 999999 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 19.46 | 352.82 | -25.57 | 54.52 | 0.5017 | -652.0 | -540.6 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 18.16 | 352.96 | -25.43 | 56.68 | 0.4902 | -899.0 | -775.9 | |
| 0.91 | -5.00 | 0.51 | -5.00 | 15.40 | 353.32 | -25.07 | 61.55 | 0.4665 | -661.0 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.77 | 17.59 | 352.83 | -25.55 | 57.83 | 0.4877 | -834.0 | -699.7 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 20.54 | 352.34 | -26.05 | 53.16 | 0.5158 | -572.0 | -458.7 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 20.38 | 352.37 | -26.02 | 53.39 | 0.5142 | -732.0 | -547.7 | |
| 3.00 | -5.00 | 1.69 | -5.00 | 16.05 | 352.95 | -25.43 | 60.60 | 0.4756 | -692.5 | 999999 | |
| 0.00 | 3.09 | 0.00 | 1.78 | 20.15 | 352.30 | -26.08 | 53.84 | 0.5133 | -792.0 | -561.9 | |
| 0.00 | 2.91 | 0.00 | 1.68 | 19.83 | 352.07 | -26.32 | 54.60 | 0.5136 | -470.0 | -383.9 | |
| 5.18 | 6.08 | 2.93 | 3.44 | 15.00 | 351.93 | -26.45 | 63.45 | 0.4829 | -800.9 | -525.8 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 21.10 | 350.14 | -28.25 | 54.22 | 0.5464 | -649.0 | -505.8 | |
| 0.00 | 7.90 | 0.00 | 4.49 | 14.58 | 351.21 | -27.17 | 64.79 | 0.4905 | -666.0 | -338.7 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 14.05 | 351.28 | -27.11 | 65.76 | 0.4867 | -798.0 | -636.6 | |
| 0.00 | 2.36 | 0.00 | 1.37 | 18.33 | 350.63 | -27.75 | 58.40 | 0.5210 | -179.0 | -353.7 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 15.50 | 350.76 | -27.62 | 63.37 | 0.5018 | 783.0 | 669.7 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 16.22 | 350.54 | -27.84 | 62.22 | 0.5088 | -599.0 | -430.7 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 15.59 | 350.57 | -27.82 | 63.35 | 0.5049 | 642.0 | 517.0 | |
| 3.45 | 23.34 | 1.97 | 13.37 | 14.75 | 350.58 | -27.80 | 64.90 | 0.5001 | 975.3 | 654.4 | |
| 0.00 | 2.72 | 0.00 | 1.56 | 13.96 | 350.08 | -28.30 | 66.72 | 0.5029 | 726.0 | 652.0 | |
| 0.00 | 3.36 | 0.00 | 1.93 | 14.76 | 349.86 | -28.52 | 65.36 | 0.5100 | 871.0 | 608.6 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 18.81 | 349.11 | -29.27 | 58.79 | 0.5432 | -632.0 | -534.8 | |
| 2.36 | 31.42 | 1.37 | 18.27 | 15.54 | 349.57 | -28.82 | 64.14 | 0.5181 | 900.2 | 800.3 | |
| 0.00 | 2.27 | 0.00 | 1.31 | 15.26 | 349.57 | -28.81 | 64.65 | 0.5165 | 863.0 | 789.2 | |
| 0.00 | 4.27 | 0.00 | 2.48 | 15.97 | 349.35 | -29.03 | 63.51 | 0.5233 | 573.0 | 521.4 | |
| 0.00 | 1.73 | 0.00 | 1.00 | 15.28 | 349.28 | -29.10 | 64.79 | 0.5206 | 703.0 | 557.3 | |
| 0.64 | -29.00 | 0.37 | -29.00 | 15.81 | 349.16 | -29.22 | 63.92 | 0.5250 | 939.0 | 999999 | |
| 10.90 | -29.00 | 6.36 | -29.00 | 15.87 | 348.83 | -29.56 | 64.05 | 0.5298 | 915.5 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 14.74 | 349.00 | -29.38 | 65.95 | 0.5217 | 738.0 | 585.6 | |
| 0.00 | 1.63 | 0.00 | 0.95 | 15.46 | 348.78 | -29.60 | 64.80 | 0.5282 | 644.0 | 539.4 | |
| 0.00 | 1.82 | 0.00 | 1.06 | 15.73 | 348.48 | -29.90 | 64.50 | 0.5337 | 731.0 | 553.1 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 16.70 | 348.24 | -30.14 | 62.97 | 0.5420 | 839.0 | 701.8 | |
| 0.00 | 2.82 | 0.00 | 1.65 | 16.17 | 348.30 | -30.08 | 63.86 | 0.5384 | 735.0 | 617.0 | |
| 0.00 | 1.54 | 0.00 | 0.92 | 17.89 | 347.77 | -30.61 | 61.28 | 0.5548 | 865.0 | 594.4 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 17.57 | 347.57 | -30.81 | 61.95 | 0.5555 | 754.0 | 523.3 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 17.69 | 347.43 | -30.95 | 61.83 | 0.5579 | 747.0 | 571.2 | |
| 11.99 | 17.80 | 7.10 | 10.54 | 16.49 | 347.50 | -30.88 | 63.80 | 0.5505 | 874.7 | 686.8 | |
| 0.00 | 3.18 | 0.00 | 1.90 | 17.81 | 347.15 | -31.24 | 61.82 | 0.5622 | 790.0 | 787.7 | |
| 0.00 | 4.99 | 0.00 | 3.00 | 18.18 | 347.00 | -31.39 | 61.30 | 0.5662 | 784.0 | 624.6 | |
| 0.00 | 3.09 | 0.00 | 1.85 | 17.55 | 347.12 | -31.26 | 62.26 | 0.5612 | 693.0 | 624.9 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 16.74 | 347.20 | -31.18 | 63.57 | 0.5558 | 541.0 | 439.5 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 17.21 | 347.11 | -31.27 | 62.84 | 0.5594 | 717.0 | 618.9 | |
| 0.00 | 2.54 | 0.00 | 1.53 | 17.96 | 346.85 | -31.53 | 61.76 | 0.5668 | 689.0 | 569.0 | |
| 0.00 | 4.45 | 0.00 | 2.67 | 17.67 | 346.72 | -31.66 | 62.32 | 0.5669 | 521.0 | 446.6 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 17.38 | 346.67 | -31.72 | 62.82 | 0.5661 | 572.0 | 395.9 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |