group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
45.04 | 210.35 | 23.83 | 111.27 | 17.13 | 20.13 | 11.02 | 328.70 | 0.3532 | -417.9 | -358.1 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
24.51 | 174.14 | 12.99 | 92.27 | 16.81 | 21.21 | 12.09 | 325.61 | 0.3565 | -1253.4 | -481.7 | |
6.15 | -1.00 | 3.27 | -1.00 | 17.20 | 21.10 | 11.99 | 326.46 | 0.3606 | -983.5 | 999999 | |
4.52 | -1.00 | 2.40 | -1.00 | 17.10 | 20.64 | 11.52 | 327.32 | 0.3552 | -983.3 | 999999 | |
0.00 | 1.18 | 0.00 | 0.62 | 18.19 | 19.77 | 10.65 | 330.92 | 0.3628 | -798.0 | -580.2 | |
0.00 | 1.36 | 0.00 | 0.72 | 18.15 | 19.57 | 10.45 | 331.33 | 0.3608 | -781.0 | -660.5 | |
0.00 | 1.18 | 0.00 | 0.62 | 16.97 | 18.50 | 9.38 | 332.19 | 0.3356 | -1005.0 | -844.3 | |
0.00 | 1.09 | 0.00 | 0.57 | 17.23 | 18.42 | 9.30 | 332.76 | 0.3386 | -700.0 | -631.2 | |
1.90 | 5.07 | 1.00 | 2.66 | 17.80 | 16.57 | 7.45 | 338.23 | 0.3345 | -988.7 | -774.0 | |
0.00 | 1.09 | 0.00 | 0.57 | 18.67 | 15.38 | 6.26 | 342.29 | 0.3412 | 767.0 | 609.0 | |
0.00 | 0.90 | 0.00 | 0.48 | 19.54 | 15.12 | 6.00 | 343.74 | 0.3536 | 809.0 | 635.6 | |
0.00 | 2.80 | 0.00 | 1.46 | 16.62 | 14.64 | 5.52 | 342.34 | 0.3053 | 918.0 | 791.6 | |
5.52 | 10.40 | 2.90 | 5.47 | 18.57 | 14.57 | 5.45 | 344.37 | 0.3359 | 1049.8 | 796.1 | |
2.44 | 3.44 | 1.27 | 1.79 | 17.32 | 14.44 | 5.32 | 343.64 | 0.3155 | 974.7 | 748.9 | |
0.00 | 1.09 | 0.00 | 0.57 | 18.99 | 14.30 | 5.18 | 345.46 | 0.3413 | 858.0 | 660.2 | |
0.00 | 1.09 | 0.00 | 0.57 | 18.28 | 14.21 | 5.09 | 345.13 | 0.3297 | 983.0 | 920.0 | |
0.00 | 2.53 | 0.00 | 1.33 | 18.95 | 14.04 | 4.92 | 346.14 | 0.3398 | 854.0 | 782.0 | |
0.00 | 1.18 | 0.00 | 0.62 | 18.63 | 14.03 | 4.91 | 345.92 | 0.3346 | 876.0 | 717.8 | |
0.00 | 1.81 | 0.00 | 0.95 | 19.47 | 13.57 | 4.45 | 347.76 | 0.3463 | 811.0 | 552.7 |
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. |
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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. |
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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. |