group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
78.74 | 334.13 | 56.20 | 238.37 | -19.01 | 337.17 | -41.04 | 120.31 | 0.7179 | 206.1 | 164.5 |
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-14 21:58:58 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 | 1.72 | 0.00 | 1.13 | -19.71 | 343.48 | -34.73 | 125.06 | 0.6575 | 717.0 | 573.1 | |
0.00 | 1.20 | 0.00 | 0.83 | -19.16 | 339.65 | -38.55 | 121.83 | 0.6953 | 290.0 | 144.1 | |
38.25 | 199.59 | 26.13 | 136.28 | -17.90 | 339.43 | -38.78 | 120.05 | 0.6909 | 1095.7 | 376.2 | |
5.59 | 83.29 | 3.87 | 58.23 | -19.06 | 338.95 | -39.25 | 121.29 | 0.7022 | 645.4 | -176.4 | |
17.71 | -4.00 | 12.44 | -4.00 | -18.93 | 337.97 | -40.24 | 120.57 | 0.7120 | -847.5 | 999999 | |
1.81 | -4.00 | 1.26 | -4.00 | -18.36 | 338.09 | -40.12 | 119.89 | 0.7077 | 374.2 | 999999 | |
2.66 | -4.00 | 1.88 | -4.00 | -18.56 | 337.70 | -40.50 | 119.94 | 0.7129 | -748.1 | 999999 | |
0.95 | -4.00 | 0.67 | -4.00 | -18.47 | 337.65 | -40.56 | 119.79 | 0.7130 | 231.0 | 999999 | |
0.00 | 2.15 | 0.00 | 1.52 | -18.44 | 337.37 | -40.84 | 119.61 | 0.7159 | -89.0 | -33.9 | |
0.00 | 0.95 | 0.00 | 0.67 | -18.80 | 337.18 | -41.03 | 119.97 | 0.7197 | -510.0 | -428.3 | |
3.95 | 4.64 | 2.79 | 3.28 | -17.69 | 337.12 | -41.08 | 118.52 | 0.7149 | 672.1 | 480.8 | |
0.00 | 0.95 | 0.00 | 0.67 | -17.56 | 336.54 | -41.67 | 118.04 | 0.7205 | 346.0 | 327.1 | |
0.00 | 1.12 | 0.00 | 0.80 | -17.28 | 336.41 | -41.80 | 117.61 | 0.7206 | 610.0 | 465.2 | |
0.00 | 1.12 | 0.00 | 0.83 | -19.39 | 334.86 | -43.34 | 119.52 | 0.7464 | 711.0 | 532.8 | |
0.00 | 0.60 | 0.00 | 0.45 | -19.09 | 334.58 | -43.63 | 119.00 | 0.7479 | 440.0 | 351.4 | |
0.00 | 1.72 | 0.00 | 1.42 | -22.83 | 330.35 | -47.86 | 121.52 | 0.8039 | -652.0 | -485.0 | |
0.00 | 0.86 | 0.00 | 0.76 | -24.81 | 328.05 | -50.16 | 122.77 | 0.8311 | -516.0 | -473.1 | |
1.89 | 2.49 | 1.57 | 2.06 | -20.98 | 329.60 | -48.61 | 119.05 | 0.8035 | 401.5 | 440.9 | |
0.00 | 6.19 | 0.00 | 5.66 | -25.29 | 326.83 | -51.38 | 122.81 | 0.8426 | -36.0 | 13.8 | |
0.00 | 0.69 | 0.00 | 0.62 | -24.44 | 327.27 | -50.94 | 122.05 | 0.8361 | -146.0 | -267.4 | |
0.00 | 1.55 | 0.00 | 1.42 | -25.07 | 326.48 | -51.72 | 122.44 | 0.8446 | -432.0 | -370.9 | |
0.00 | 1.55 | 0.00 | 1.42 | -24.91 | 326.42 | -51.78 | 122.23 | 0.8445 | -446.0 | -394.1 | |
0.00 | 1.20 | 0.00 | 1.14 | -25.89 | 325.50 | -52.71 | 122.94 | 0.8550 | -451.0 | -354.2 | |
0.00 | 1.38 | 0.00 | 1.27 | -24.66 | 325.98 | -52.22 | 121.79 | 0.8472 | -393.0 | -368.3 | |
0.00 | 1.63 | 0.00 | 1.54 | -25.22 | 325.43 | -52.78 | 122.19 | 0.8534 | -422.0 | -400.8 | |
0.00 | 1.12 | 0.00 | 0.97 | -20.79 | 327.16 | -51.04 | 117.87 | 0.8246 | -634.0 | -515.8 | |
1.20 | 2.06 | 1.10 | 1.89 | -22.82 | 325.81 | -52.40 | 119.68 | 0.8426 | -599.8 | -412.7 | |
0.00 | 1.29 | 0.00 | 1.20 | -23.64 | 325.24 | -52.96 | 120.37 | 0.8497 | -432.0 | -353.3 | |
4.73 | 7.31 | 4.49 | 6.94 | -24.12 | 324.74 | -53.47 | 120.72 | 0.8552 | -376.2 | -109.3 | |
0.00 | 1.29 | 0.00 | 1.20 | -23.44 | 325.14 | -53.07 | 120.12 | 0.8500 | -384.0 | -317.9 | |
0.00 | 1.20 | 0.00 | 1.12 | -23.02 | 325.11 | -53.09 | 119.64 | 0.8488 | -518.0 | -365.0 | |
0.00 | 1.38 | 0.00 | 1.29 | -23.29 | 324.96 | -53.25 | 119.88 | 0.8509 | -347.0 | -217.9 | |
0.00 | 1.89 | 0.00 | 1.76 | -22.76 | 324.93 | -53.27 | 119.29 | 0.8495 | -341.0 | -281.5 |
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. |