SDO HMI 2014-07-12 10:00:40 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 |
| 60.14 | 171.09 | 30.15 | 85.89 | 7.83 | 162.86 | -6.79 | 147.28 | 0.1418 | -355.2 | -260.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-12 10:00:40 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 | 2.18 | 0.00 | 1.08 | 8.55 | 170.78 | 1.13 | 346.02 | 0.0811 | -1036.0 | -898.3 | |
| 0.00 | 2.09 | 0.00 | 1.04 | 8.24 | 170.41 | 0.76 | 349.82 | 0.0745 | -919.0 | -704.0 | |
| 0.00 | 1.82 | 0.00 | 0.90 | 7.91 | 170.26 | 0.60 | 351.16 | 0.0683 | -1039.0 | -774.3 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 8.09 | 170.20 | 0.54 | 352.40 | 0.0713 | -928.0 | -764.3 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 8.03 | 169.67 | 0.02 | 359.71 | 0.0696 | -943.0 | -700.8 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 8.21 | 169.61 | -0.04 | 0.56 | 0.0728 | -948.0 | -752.4 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 7.91 | 169.55 | -0.10 | 1.52 | 0.0675 | -983.0 | -823.0 | |
| 0.00 | 2.54 | 0.00 | 1.26 | 8.61 | 169.24 | -0.41 | 5.10 | 0.0801 | -855.0 | -719.4 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 8.34 | 169.24 | -0.41 | 5.43 | 0.0753 | -1042.0 | -841.1 | |
| 11.54 | 15.08 | 5.72 | 7.48 | 5.96 | 168.38 | -1.27 | 33.59 | 0.0400 | -1176.3 | -665.4 | |
| 0.36 | 2.36 | 0.18 | 1.17 | 6.20 | 167.86 | -1.79 | 39.68 | 0.0489 | -1175.0 | -973.5 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 6.75 | 167.74 | -1.91 | 35.21 | 0.0578 | -909.0 | -703.3 | |
| 0.00 | 5.45 | 0.00 | 2.70 | 6.50 | 167.71 | -1.94 | 38.26 | 0.0547 | -1174.0 | -935.2 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 8.18 | 167.67 | -1.98 | 25.41 | 0.0801 | -873.0 | -717.1 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 6.63 | 167.55 | -2.10 | 39.02 | 0.0580 | -864.0 | -706.9 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 9.22 | 167.05 | -2.60 | 26.45 | 0.1011 | 903.0 | 680.8 | |
| 0.00 | 2.45 | 0.00 | 1.22 | 6.26 | 166.67 | -2.99 | 53.36 | 0.0649 | -851.0 | -833.8 | |
| 0.00 | 4.63 | 0.00 | 2.30 | 6.90 | 166.45 | -3.21 | 48.16 | 0.0749 | -900.0 | -756.0 | |
| 1.82 | 3.54 | 0.90 | 1.76 | 9.04 | 166.40 | -3.25 | 32.79 | 0.1039 | 1128.7 | 844.5 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 4.58 | 165.84 | -3.81 | 82.00 | 0.0672 | 992.0 | 778.6 | |
| 1.54 | 3.27 | 0.77 | 1.62 | 5.07 | 165.41 | -4.24 | 76.40 | 0.0761 | 1209.6 | 936.6 | |
| 3.45 | 18.53 | 1.72 | 9.23 | 7.99 | 165.24 | -4.41 | 47.90 | 0.1032 | -1243.7 | -743.7 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 7.08 | 165.25 | -4.41 | 55.24 | 0.0932 | -948.0 | -771.4 | |
| 8.45 | -22.00 | 4.21 | -22.00 | 8.18 | 165.20 | -4.45 | 46.81 | 0.1058 | -1114.0 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 5.13 | 165.14 | -4.52 | 76.46 | 0.0810 | 886.0 | 640.0 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 4.79 | 164.89 | -4.76 | 81.03 | 0.0841 | 970.0 | 804.5 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 6.58 | 164.23 | -5.42 | 64.66 | 0.1043 | 916.0 | 699.2 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 8.93 | 164.02 | -5.63 | 48.63 | 0.1298 | -873.0 | -620.9 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 10.24 | 163.07 | -6.59 | 46.19 | 0.1571 | 859.0 | 622.8 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 6.88 | 162.87 | -6.78 | 66.99 | 0.1279 | -948.0 | -700.6 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.29 | 162.80 | -6.85 | 52.05 | 0.1499 | -716.0 | -507.5 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 4.62 | 162.84 | -6.82 | 84.96 | 0.1193 | -772.0 | -516.8 | |
| 0.00 | 2.36 | 0.00 | 1.18 | 2.27 | 162.17 | -7.48 | 103.20 | 0.1342 | -861.0 | -692.7 | |
| 0.00 | 2.72 | 0.00 | 1.37 | 10.27 | 162.00 | -7.65 | 50.27 | 0.1710 | 953.0 | 731.8 | |
| 0.00 | 3.00 | 0.00 | 1.50 | 3.92 | 162.01 | -7.64 | 90.77 | 0.1333 | -814.0 | -789.2 | |
| 0.00 | 2.18 | 0.00 | 1.10 | 10.66 | 161.27 | -8.38 | 51.05 | 0.1850 | 759.0 | 563.9 | |
| 3.54 | 43.33 | 1.78 | 21.80 | 8.02 | 160.71 | -8.94 | 65.53 | 0.1698 | -1115.4 | -735.9 | |
| 11.54 | -37.00 | 5.80 | -37.00 | 8.42 | 160.67 | -8.98 | 63.51 | 0.1733 | -1153.6 | 999999 | |
| 4.00 | -37.00 | 2.01 | -37.00 | 8.20 | 160.46 | -9.19 | 65.15 | 0.1750 | -1074.9 | 999999 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 10.80 | 160.27 | -9.39 | 53.52 | 0.2001 | -730.0 | -549.7 | |
| 2.91 | -37.00 | 1.46 | -37.00 | 8.26 | 160.30 | -9.35 | 65.20 | 0.1779 | -920.5 | 999999 | |
| 2.72 | -37.00 | 1.37 | -37.00 | 8.35 | 160.02 | -9.63 | 65.37 | 0.1830 | -853.9 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 7.78 | 158.28 | -11.37 | 71.24 | 0.2073 | 742.0 | 594.2 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 7.98 | 157.43 | -12.23 | 71.52 | 0.2221 | 911.0 | 567.7 | |
| 0.00 | 2.00 | 0.00 | 1.02 | 8.93 | 156.95 | -12.70 | 68.26 | 0.2348 | 1037.0 | 914.9 | |
| 0.00 | 2.36 | 0.00 | 1.20 | 8.74 | 156.87 | -12.79 | 69.13 | 0.2352 | 923.0 | 707.9 | |
| 0.64 | 2.45 | 0.32 | 1.25 | 9.59 | 156.52 | -13.13 | 66.31 | 0.2458 | 1057.9 | 880.3 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 7.08 | 156.35 | -13.30 | 76.53 | 0.2359 | 730.0 | 612.3 | |
| 0.73 | 2.27 | 0.37 | 1.16 | 7.38 | 156.09 | -13.56 | 75.53 | 0.2413 | 1031.2 | 862.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 9.09 | 155.93 | -13.72 | 69.02 | 0.2519 | 909.0 | 730.2 | |
| 6.90 | 9.08 | 3.54 | 4.66 | 9.36 | 155.29 | -14.37 | 68.87 | 0.2636 | 1052.6 | 717.2 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 11.75 | 153.46 | -16.19 | 63.40 | 0.3066 | 819.0 | 666.4 | |
| 0.00 | 2.18 | 0.00 | 1.15 | 9.34 | 149.72 | -19.93 | 74.02 | 0.3513 | 639.0 | 532.3 | |
| 0.00 | 2.00 | 0.00 | 1.07 | 10.60 | 148.52 | -21.13 | 71.48 | 0.3753 | 808.0 | 704.0 | |
| 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. | |