SDO HMI 2014-11-06 20:00:28 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.60 | 107.70 | 23.91 | 61.54 | -4.93 | 87.34 | 28.43 | 252.87 | 0.4976 | 17.5 | -37.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-06 20:00:28 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 | 1.64 | 0.00 | 0.99 | -5.43 | 92.25 | 33.35 | 254.71 | 0.5696 | 517.0 | 500.1 | |
| 0.00 | 1.29 | 0.00 | 0.78 | -7.24 | 91.63 | 32.73 | 251.33 | 0.5684 | 717.0 | 555.5 | |
| 7.16 | 32.19 | 4.26 | 19.09 | -4.80 | 91.40 | 32.50 | 255.42 | 0.5553 | 748.5 | 494.8 | |
| 12.17 | -3.00 | 7.20 | -3.00 | -4.51 | 91.03 | 32.13 | 255.76 | 0.5491 | 942.0 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.35 | -3.15 | 90.55 | 31.65 | 258.02 | 0.5378 | 486.0 | 354.3 | |
| 0.00 | 1.73 | 0.00 | 1.01 | -4.50 | 90.01 | 31.11 | 255.31 | 0.5346 | 782.0 | 644.9 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -3.66 | 89.87 | 30.97 | 256.80 | 0.5296 | 501.0 | 562.4 | |
| 0.00 | 0.60 | 0.00 | 0.35 | -4.97 | 89.58 | 30.68 | 254.26 | 0.5303 | 687.0 | 574.3 | |
| 0.00 | 1.21 | 0.00 | 0.70 | -0.53 | 89.29 | 30.39 | 262.50 | 0.5123 | 606.0 | 450.6 | |
| 0.00 | 0.26 | 0.00 | 0.15 | -6.20 | 89.41 | 30.51 | 251.94 | 0.5330 | 542.0 | 528.3 | |
| 0.00 | 1.81 | 0.00 | 1.05 | -5.35 | 89.22 | 30.32 | 253.38 | 0.5267 | 794.0 | 725.1 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -5.98 | 89.19 | 30.29 | 252.21 | 0.5289 | 595.0 | 500.7 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -6.58 | 89.16 | 30.26 | 251.11 | 0.5312 | 588.0 | 432.3 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -6.66 | 88.89 | 29.98 | 250.80 | 0.5277 | 747.0 | 519.1 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -3.10 | 87.52 | 28.62 | 256.80 | 0.4933 | 773.0 | 654.1 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -3.90 | 87.24 | 28.34 | 255.08 | 0.4921 | 714.0 | 557.6 | |
| 0.00 | 1.55 | 0.00 | 0.88 | -4.14 | 87.18 | 28.28 | 254.59 | 0.4922 | 696.0 | 517.0 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -6.83 | 86.74 | 27.84 | 249.11 | 0.4983 | -743.0 | -587.7 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -5.07 | 86.31 | 27.41 | 252.24 | 0.4834 | -549.0 | -505.3 | |
| 6.13 | 11.13 | 3.45 | 6.28 | -5.77 | 85.81 | 26.90 | 250.51 | 0.4795 | -932.1 | -625.7 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -5.05 | 85.77 | 26.87 | 251.93 | 0.4755 | -681.0 | -531.2 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -4.75 | 85.76 | 26.86 | 252.53 | 0.4739 | -443.0 | -353.6 | |
| 0.78 | 1.73 | 0.44 | 0.97 | -5.92 | 85.48 | 26.58 | 250.01 | 0.4755 | -833.4 | -764.9 | |
| 2.33 | 4.66 | 1.30 | 2.61 | -4.80 | 85.33 | 26.42 | 252.16 | 0.4678 | -843.6 | -575.7 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -5.06 | 85.17 | 26.27 | 251.52 | 0.4668 | -722.0 | -594.5 | |
| 5.18 | 30.12 | 2.89 | 16.77 | -4.76 | 84.93 | 26.02 | 251.99 | 0.4617 | -1017.8 | -544.1 | |
| 7.85 | -26.00 | 4.37 | -26.00 | -4.72 | 84.63 | 25.72 | 251.87 | 0.4571 | -1169.1 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -6.59 | 80.50 | 21.59 | 244.32 | 0.4074 | -675.0 | -624.5 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -8.97 | 79.01 | 20.11 | 237.40 | 0.4049 | -785.0 | -633.5 | |
| 0.00 | 1.73 | 0.00 | 0.93 | -8.75 | 78.42 | 19.52 | 237.11 | 0.3950 | -692.0 | -597.9 | |
| 0.00 | 2.85 | 0.00 | 1.50 | -2.98 | 78.09 | 19.19 | 250.77 | 0.3492 | -6.0 | 3.8 | |
| 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. | |