group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
38.50 | 81.80 | 22.22 | 47.23 | 14.24 | 301.53 | -30.32 | 72.89 | 0.5138 | -138.1 | -25.8 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
13.26 | 17.95 | 7.51 | 10.18 | 14.09 | 303.34 | -28.51 | 72.48 | 0.4874 | -893.0 | -669.8 | |
0.00 | 1.17 | 0.00 | 0.67 | 14.52 | 302.78 | -29.07 | 71.86 | 0.4969 | 648.0 | 553.6 | |
1.53 | 3.34 | 0.88 | 1.91 | 14.10 | 302.41 | -29.44 | 72.84 | 0.5009 | -898.6 | -610.0 | |
4.24 | 10.19 | 2.43 | 5.85 | 14.30 | 302.16 | -29.69 | 72.54 | 0.5051 | -886.8 | -768.9 | |
0.36 | 1.89 | 0.21 | 1.09 | 13.63 | 301.75 | -30.10 | 74.00 | 0.5090 | -671.5 | -537.6 | |
3.97 | 10.73 | 2.29 | 6.20 | 14.42 | 301.49 | -30.36 | 72.58 | 0.5150 | -809.1 | -644.4 | |
0.00 | 0.99 | 0.00 | 0.58 | 14.98 | 301.01 | -30.85 | 71.72 | 0.5237 | 665.0 | 510.8 | |
1.80 | 2.44 | 1.05 | 1.41 | 14.55 | 301.04 | -30.81 | 72.51 | 0.5219 | -543.3 | -488.3 | |
0.00 | 4.96 | 0.00 | 2.87 | 13.63 | 301.10 | -30.75 | 74.23 | 0.5183 | 541.0 | 602.5 | |
1.08 | 11.55 | 0.63 | 6.71 | 13.61 | 300.81 | -31.04 | 74.36 | 0.5224 | 826.1 | 589.0 | |
1.26 | 1.53 | 0.74 | 0.90 | 14.75 | 300.20 | -31.65 | 72.45 | 0.5343 | 829.9 | 614.7 | |
0.00 | 1.26 | 0.00 | 0.74 | 14.73 | 299.94 | -31.91 | 72.57 | 0.5379 | 730.0 | 623.1 | |
9.29 | 11.82 | 5.47 | 6.95 | 15.06 | 299.70 | -32.15 | 72.07 | 0.5422 | 854.0 | 637.0 | |
1.71 | 1.98 | 1.01 | 1.17 | 13.84 | 299.42 | -32.44 | 74.38 | 0.5429 | 733.0 | 526.3 |
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. |