group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
11.64 | 72.06 | 7.41 | 44.60 | -10.16 | 358.23 | 36.96 | 262.30 | 0.5995 | 297.9 | 332.0 |
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-14 00:00:29 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 |
3.91 | 5.73 | 2.52 | 3.69 | -7.86 | 1.43 | 40.15 | 266.35 | 0.6424 | 640.2 | 486.7 | |
0.00 | 3.82 | 0.00 | 2.46 | -7.31 | 1.21 | 39.93 | 267.22 | 0.6397 | 656.0 | 499.5 | |
0.00 | 1.22 | 0.00 | 0.78 | -7.39 | 0.94 | 39.67 | 267.11 | 0.6361 | 376.0 | 399.4 | |
0.00 | 1.22 | 0.00 | 0.78 | -7.87 | 0.96 | 39.68 | 266.36 | 0.6361 | 658.0 | 574.7 | |
0.00 | 1.65 | 0.00 | 1.06 | -6.80 | 0.85 | 39.57 | 268.05 | 0.6352 | 549.0 | 471.8 | |
0.00 | 1.13 | 0.00 | 0.72 | -6.21 | 0.44 | 39.16 | 269.03 | 0.6302 | 546.0 | 474.2 | |
0.00 | 2.00 | 0.00 | 1.27 | -7.49 | 0.52 | 39.25 | 266.99 | 0.6304 | 572.0 | 493.1 | |
0.00 | 3.73 | 0.00 | 2.37 | -7.05 | 0.29 | 39.01 | 267.69 | 0.6275 | 714.0 | 556.7 | |
0.00 | 0.78 | 0.00 | 0.50 | -12.94 | 1.05 | 39.78 | 258.38 | 0.6389 | 618.0 | 523.0 | |
0.00 | 0.95 | 0.00 | 0.60 | -8.92 | 0.11 | 38.83 | 264.70 | 0.6244 | 129.0 | 212.3 | |
7.73 | 16.58 | 4.89 | 10.49 | -9.76 | 0.18 | 38.90 | 263.36 | 0.6254 | 796.4 | 494.6 | |
0.00 | 4.77 | 0.00 | 3.01 | -9.19 | 359.83 | 38.55 | 264.28 | 0.6206 | 969.0 | 705.9 | |
0.00 | 1.30 | 0.00 | 0.81 | -8.58 | 359.10 | 37.83 | 265.28 | 0.6107 | 744.0 | 661.9 | |
0.00 | 2.95 | 0.00 | 1.85 | -13.14 | 359.24 | 37.96 | 257.83 | 0.6151 | 803.0 | 608.6 | |
0.00 | 1.22 | 0.00 | 0.74 | -11.01 | 357.48 | 36.20 | 261.16 | 0.5890 | 711.0 | 626.3 | |
0.00 | 0.95 | 0.00 | 0.58 | -10.88 | 357.24 | 35.96 | 261.37 | 0.5855 | 629.0 | 519.5 | |
0.00 | 2.26 | 0.00 | 1.37 | -11.06 | 357.11 | 35.83 | 261.03 | 0.5839 | 728.0 | 608.2 | |
0.00 | 1.91 | 0.00 | 1.16 | -11.44 | 356.86 | 35.59 | 260.36 | 0.5808 | 662.0 | 532.5 | |
0.00 | 1.04 | 0.00 | 0.63 | -11.84 | 356.74 | 35.46 | 259.65 | 0.5794 | 694.0 | 527.5 | |
0.00 | 1.04 | 0.00 | 0.63 | -12.79 | 356.10 | 34.82 | 257.91 | 0.5716 | 539.0 | 433.0 | |
0.00 | 0.95 | 0.00 | 0.58 | -15.48 | 356.08 | 34.80 | 253.25 | 0.5766 | 531.0 | 445.5 | |
0.00 | 1.82 | 0.00 | 1.09 | -14.72 | 355.22 | 33.95 | 254.33 | 0.5631 | 746.0 | 615.4 | |
0.00 | 0.78 | 0.00 | 0.45 | -14.03 | 352.34 | 31.06 | 254.76 | 0.5208 | -591.0 | -505.2 | |
0.00 | 1.13 | 0.00 | 0.65 | -10.67 | 351.76 | 30.48 | 261.16 | 0.5065 | -593.0 | -477.4 | |
0.00 | 1.22 | 0.00 | 0.70 | -9.72 | 351.66 | 30.38 | 263.04 | 0.5043 | -552.0 | -398.7 | |
0.00 | 0.87 | 0.00 | 0.50 | -13.19 | 351.86 | 30.58 | 256.25 | 0.5120 | -627.0 | -544.9 | |
0.00 | 1.56 | 0.00 | 0.90 | -13.97 | 351.36 | 30.09 | 254.58 | 0.5067 | -388.0 | -394.9 | |
0.00 | 1.22 | 0.00 | 0.70 | -15.53 | 351.49 | 30.22 | 251.60 | 0.5131 | -669.0 | -582.9 | |
0.00 | 1.91 | 0.00 | 1.09 | -14.10 | 351.20 | 29.93 | 254.27 | 0.5047 | -585.0 | -449.3 | |
0.00 | 1.22 | 0.00 | 0.69 | -10.68 | 350.67 | 29.40 | 260.99 | 0.4904 | -622.0 | -554.9 | |
0.00 | 1.22 | 0.00 | 0.69 | -16.02 | 350.46 | 29.19 | 250.23 | 0.5001 | -692.0 | -509.9 | |
0.00 | 0.69 | 0.00 | 0.39 | -16.29 | 349.90 | 28.63 | 249.42 | 0.4932 | -624.0 | -509.5 | |
0.00 | 1.22 | 0.00 | 0.67 | -13.98 | 346.81 | 25.53 | 252.74 | 0.4398 | -698.0 | -617.9 |
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. |