| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 172.43 | 846.51 | 97.13 | 476.81 | 15.92 | 61.31 | -27.24 | 68.57 | 0.4743 | -172.1 | -113.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-08-19 17:59:09 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 | 0.90 | 0.00 | 0.48 | 15.97 | 69.04 | -19.51 | 62.72 | 0.3629 | -905.0 | -736.5 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 15.46 | 67.78 | -20.77 | 65.23 | 0.3780 | -782.0 | -645.8 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 13.88 | 66.69 | -21.85 | 70.04 | 0.3861 | -787.0 | -619.9 | |
| 15.38 | 306.53 | 8.39 | 167.72 | 15.49 | 64.85 | -23.70 | 67.51 | 0.4209 | -1488.9 | -432.7 | |
| 4.32 | -4.00 | 2.36 | -4.00 | 15.82 | 64.77 | -23.77 | 66.81 | 0.4237 | -1187.5 | 999999 | |
| 1.98 | 3.42 | 1.07 | 1.86 | 12.73 | 64.81 | -23.73 | 73.99 | 0.4102 | -979.0 | -797.9 | |
| 25.36 | -4.00 | 13.90 | -4.00 | 15.65 | 64.35 | -24.20 | 67.50 | 0.4290 | -1078.5 | 999999 | |
| 1.44 | 2.34 | 0.78 | 1.27 | 12.72 | 64.54 | -24.01 | 74.15 | 0.4143 | -708.2 | -621.5 | |
| 11.51 | -4.00 | 6.32 | -4.00 | 15.21 | 64.06 | -24.49 | 68.68 | 0.4312 | -960.8 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 17.18 | 63.41 | -25.14 | 64.86 | 0.4502 | 591.0 | 346.1 | |
| 0.90 | -4.00 | 0.49 | -4.00 | 15.13 | 63.65 | -24.90 | 69.12 | 0.4368 | -400.6 | 999999 | |
| 0.00 | 2.16 | 0.00 | 1.19 | 15.98 | 63.47 | -25.08 | 67.37 | 0.4433 | -717.0 | -444.8 | |
| 0.00 | 2.25 | 0.00 | 1.25 | 16.46 | 63.23 | -25.32 | 66.50 | 0.4490 | -749.0 | -619.6 | |
| 2.07 | 3.51 | 1.14 | 1.94 | 15.13 | 63.20 | -25.35 | 69.37 | 0.4434 | -620.9 | -448.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 19.19 | 62.60 | -25.95 | 61.39 | 0.4727 | 531.0 | 494.7 | |
| 10.25 | 12.95 | 5.75 | 7.26 | 18.56 | 62.52 | -26.03 | 62.68 | 0.4701 | -887.1 | -679.7 | |
| 0.00 | 2.16 | 0.00 | 1.22 | 20.33 | 62.18 | -26.37 | 59.53 | 0.4852 | -764.0 | -533.5 | |
| 1.89 | 239.34 | 1.05 | 134.05 | 16.30 | 62.59 | -25.96 | 67.25 | 0.4575 | 272.8 | -327.5 | |
| 26.71 | -18.00 | 14.91 | -18.00 | 16.98 | 62.42 | -26.13 | 65.96 | 0.4631 | -1265.5 | 999999 | |
| 16.64 | -18.00 | 9.34 | -18.00 | 17.70 | 62.06 | -26.49 | 64.73 | 0.4718 | -951.1 | 999999 | |
| 0.00 | 2.25 | 0.00 | 1.26 | 15.92 | 61.65 | -26.89 | 68.61 | 0.4691 | 708.0 | 535.9 | |
| 0.00 | 1.71 | 0.00 | 0.97 | 17.33 | 60.40 | -28.15 | 66.50 | 0.4931 | 369.0 | 460.8 | |
| 0.00 | 0.27 | 0.00 | 0.15 | 16.17 | 60.08 | -28.47 | 68.95 | 0.4925 | 678.0 | 599.3 | |
| 0.00 | 1.89 | 0.00 | 1.08 | 16.19 | 59.83 | -28.72 | 69.04 | 0.4962 | 894.0 | 693.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 19.57 | 59.22 | -29.33 | 63.01 | 0.5200 | -599.0 | -462.4 | |
| 0.00 | 2.79 | 0.00 | 1.61 | 17.84 | 58.92 | -29.62 | 66.37 | 0.5156 | 667.0 | 637.3 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 14.50 | 59.43 | -29.11 | 72.54 | 0.4958 | 938.0 | 850.7 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 14.55 | 59.21 | -29.34 | 72.53 | 0.4991 | 830.0 | 677.6 | |
| 0.00 | 1.62 | 0.00 | 0.93 | 15.74 | 58.99 | -29.56 | 70.31 | 0.5063 | 825.0 | 745.4 | |
| 2.43 | 5.76 | 1.39 | 3.30 | 15.53 | 58.99 | -29.56 | 70.73 | 0.5055 | 973.6 | 561.8 | |
| 0.00 | 1.35 | 0.00 | 0.77 | 14.64 | 59.09 | -29.46 | 72.41 | 0.5011 | 733.0 | 661.7 | |
| 0.00 | 3.60 | 0.00 | 2.06 | 14.94 | 59.01 | -29.54 | 71.85 | 0.5033 | 742.0 | 668.7 | |
| 2.52 | 3.06 | 1.44 | 1.75 | 13.81 | 59.03 | -29.52 | 74.07 | 0.4995 | 867.0 | 888.8 | |
| 3.15 | 9.35 | 1.81 | 5.37 | 15.14 | 58.76 | -29.79 | 71.57 | 0.5075 | 986.3 | 883.9 | |
| 0.00 | 2.25 | 0.00 | 1.29 | 15.69 | 58.64 | -29.91 | 70.57 | 0.5111 | 749.0 | 623.4 | |
| 0.00 | 0.72 | 0.00 | 0.41 | 13.59 | 58.95 | -29.60 | 74.53 | 0.5001 | 631.0 | 566.0 | |
| 0.00 | 1.80 | 0.00 | 1.04 | 15.52 | 58.41 | -30.14 | 70.99 | 0.5137 | 761.0 | 632.2 | |
| 0.00 | 1.17 | 0.00 | 0.69 | 20.23 | 57.05 | -31.49 | 63.14 | 0.5516 | 792.0 | 582.2 | |
| 0.00 | 1.35 | 0.00 | 0.80 | 19.92 | 57.05 | -31.50 | 63.68 | 0.5502 | 815.0 | 701.1 | |
| 0.00 | 1.17 | 0.00 | 0.70 | 20.39 | 56.64 | -31.91 | 63.09 | 0.5578 | 697.0 | 587.4 | |
| 1.53 | 3.15 | 0.90 | 1.86 | 18.62 | 56.80 | -31.75 | 66.07 | 0.5476 | -511.4 | -253.4 | |
| 2.97 | 4.41 | 1.77 | 2.63 | 20.07 | 56.44 | -32.10 | 63.75 | 0.5587 | 920.5 | 739.2 | |
| 5.67 | 7.83 | 3.38 | 4.67 | 19.87 | 56.26 | -32.29 | 64.19 | 0.5602 | 964.9 | 710.0 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 16.45 | 56.81 | -31.73 | 69.94 | 0.5391 | 823.0 | 719.7 | |
| 0.00 | 1.17 | 0.00 | 0.70 | 19.51 | 55.96 | -32.59 | 64.96 | 0.5625 | 660.0 | 707.1 | |
| 0.00 | 1.53 | 0.00 | 0.90 | 16.53 | 56.58 | -31.97 | 69.90 | 0.5427 | 620.0 | 476.3 | |
| 0.00 | 1.62 | 0.00 | 0.97 | 20.05 | 55.72 | -32.83 | 64.15 | 0.5680 | 725.0 | 598.8 | |
| 0.00 | 1.35 | 0.00 | 0.81 | 19.47 | 55.82 | -32.73 | 65.10 | 0.5642 | 594.0 | 624.9 | |
| 0.90 | 5.22 | 0.54 | 3.13 | 19.80 | 55.70 | -32.85 | 64.59 | 0.5671 | 836.1 | 663.1 | |
| 0.00 | 1.35 | 0.00 | 0.82 | 20.69 | 55.33 | -33.22 | 63.29 | 0.5758 | 694.0 | 568.3 | |
| 0.00 | 1.35 | 0.00 | 0.81 | 19.95 | 55.47 | -33.07 | 64.46 | 0.5707 | 754.0 | 601.0 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 20.87 | 55.25 | -33.30 | 63.03 | 0.5777 | 630.0 | 536.6 | |
| 34.81 | 186.90 | 20.40 | 109.61 | 14.12 | 56.51 | -32.04 | 74.31 | 0.5365 | 1195.3 | 391.0 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 18.81 | 55.39 | -33.16 | 66.41 | 0.5671 | 710.0 | 585.1 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 20.89 | 54.42 | -34.12 | 63.43 | 0.5882 | 597.0 | 492.3 | |
| 0.00 | 1.44 | 0.00 | 0.90 | 19.98 | 52.16 | -36.39 | 65.90 | 0.6130 | 635.0 | 439.1 | |
| 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. | |