group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
32.99 | 200.13 | 32.09 | 198.98 | 13.91 | 54.42 | -60.76 | 77.66 | 0.8674 | -88.6 | 85.5 |
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-12 18:00:39 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 |
11.99 | 63.75 | 10.46 | 55.65 | 13.81 | 59.28 | -55.90 | 77.69 | 0.8252 | -870.2 | -279.8 | |
5.23 | 7.66 | 4.71 | 6.90 | 13.82 | 58.08 | -57.11 | 77.71 | 0.8366 | -499.2 | -290.7 | |
0.99 | 5.32 | 0.92 | 4.92 | 12.30 | 57.05 | -58.13 | 79.54 | 0.8459 | -697.8 | -582.9 | |
0.00 | 2.34 | 0.00 | 2.21 | 14.21 | 56.25 | -58.93 | 77.29 | 0.8532 | -572.0 | -514.7 | |
0.00 | 0.90 | 0.00 | 0.83 | 11.67 | 57.21 | -57.98 | 80.29 | 0.8445 | -620.0 | -535.0 | |
0.00 | 1.17 | 0.00 | 1.10 | 13.81 | 56.30 | -58.89 | 77.76 | 0.8528 | -505.0 | -411.8 | |
0.00 | 0.99 | 0.00 | 0.94 | 13.26 | 56.03 | -59.15 | 78.42 | 0.8551 | -546.0 | -514.6 | |
0.00 | 0.27 | 0.00 | 0.26 | 13.54 | 55.79 | -59.39 | 78.08 | 0.8572 | -422.0 | -418.0 | |
0.00 | 3.07 | 0.00 | 2.94 | 13.25 | 55.66 | -59.52 | 78.42 | 0.8583 | -502.0 | -402.3 | |
0.00 | 0.27 | 0.00 | 0.26 | 14.21 | 55.26 | -59.92 | 77.31 | 0.8619 | -301.0 | -279.0 | |
0.72 | 5.41 | 0.70 | 5.26 | 13.53 | 55.04 | -60.14 | 78.10 | 0.8637 | -75.6 | -255.9 | |
0.00 | 1.26 | 0.00 | 1.21 | 12.04 | 55.57 | -59.61 | 79.84 | 0.8591 | -593.0 | -434.2 | |
0.00 | 1.35 | 0.00 | 1.33 | 13.63 | 54.75 | -60.43 | 77.99 | 0.8662 | 22.0 | 110.0 | |
0.00 | 2.34 | 0.00 | 2.30 | 13.30 | 54.83 | -60.36 | 78.38 | 0.8655 | 281.0 | 244.1 | |
0.00 | 1.44 | 0.00 | 1.40 | 11.77 | 55.36 | -59.83 | 80.15 | 0.8610 | -499.0 | -391.4 | |
0.54 | 2.07 | 0.53 | 2.02 | 12.03 | 55.20 | -59.99 | 79.85 | 0.8624 | -388.3 | -309.9 | |
0.00 | 1.35 | 0.00 | 1.33 | 11.99 | 54.77 | -60.41 | 79.89 | 0.8660 | -229.0 | -215.0 | |
0.00 | 0.27 | 0.00 | 0.28 | 14.47 | 53.18 | -62.00 | 77.03 | 0.8792 | 419.0 | 453.3 | |
0.00 | 1.80 | 0.00 | 1.81 | 12.03 | 54.18 | -61.00 | 79.84 | 0.8710 | -429.0 | -283.0 | |
0.45 | 3.79 | 0.46 | 3.86 | 12.06 | 53.58 | -61.60 | 79.79 | 0.8760 | -228.4 | -133.9 | |
1.53 | 4.60 | 1.62 | 4.85 | 13.10 | 52.47 | -62.71 | 78.60 | 0.8849 | 646.9 | 620.6 | |
0.90 | 1.80 | 0.93 | 1.87 | 11.70 | 53.06 | -62.12 | 80.20 | 0.8804 | -247.6 | -209.7 | |
3.61 | 36.43 | 3.96 | 39.87 | 14.82 | 51.27 | -63.92 | 76.66 | 0.8942 | 785.2 | 471.8 | |
0.36 | 3.52 | 0.39 | 3.77 | 13.54 | 51.92 | -63.27 | 78.09 | 0.8892 | 596.8 | 561.2 | |
2.98 | -23.00 | 3.29 | -23.00 | 15.14 | 51.02 | -64.17 | 76.30 | 0.8961 | 680.8 | 999999 | |
0.00 | 1.71 | 0.00 | 1.83 | 13.03 | 52.09 | -63.10 | 78.67 | 0.8880 | 510.0 | 429.4 | |
0.99 | 13.98 | 1.09 | 15.22 | 14.33 | 51.38 | -63.80 | 77.21 | 0.8933 | 735.3 | 529.4 | |
0.00 | 1.71 | 0.00 | 1.93 | 15.54 | 50.41 | -64.77 | 75.85 | 0.9006 | 605.0 | 491.3 | |
0.00 | 0.99 | 0.00 | 1.11 | 14.86 | 50.73 | -64.45 | 76.61 | 0.8982 | 405.0 | 310.5 | |
0.00 | 1.26 | 0.00 | 1.42 | 15.33 | 50.46 | -64.72 | 76.09 | 0.9002 | 356.0 | 391.9 | |
1.17 | 14.52 | 1.28 | 15.67 | 13.00 | 51.54 | -63.65 | 78.69 | 0.8922 | 497.0 | 295.1 | |
0.54 | 2.34 | 0.62 | 2.69 | 15.78 | 49.90 | -65.29 | 75.60 | 0.9044 | 367.0 | 259.0 | |
0.00 | 3.07 | 0.00 | 3.46 | 14.58 | 50.45 | -64.74 | 76.92 | 0.9004 | 512.0 | 377.6 | |
0.00 | 1.89 | 0.00 | 2.17 | 15.10 | 50.00 | -65.18 | 76.35 | 0.9036 | 482.0 | 418.8 | |
0.00 | 0.45 | 0.00 | 0.53 | 15.68 | 49.57 | -65.61 | 75.70 | 0.9067 | 10.0 | -48.6 | |
0.63 | 2.16 | 0.72 | 2.49 | 14.84 | 49.99 | -65.19 | 76.63 | 0.9036 | 318.7 | 199.3 | |
0.00 | 1.53 | 0.00 | 1.74 | 13.77 | 50.21 | -64.98 | 77.82 | 0.9021 | 251.0 | 165.6 | |
0.36 | 1.35 | 0.41 | 1.55 | 14.21 | 49.90 | -65.29 | 77.33 | 0.9044 | 75.2 | 54.2 |
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. |