St.
Pierre & Miquelon
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Date |
FP Sunrise Time (UTC) |
October 23 |
1020 |
October 24 |
1021 |
October 25 |
1023 |
October 26 |
1024 |
October 27 |
1026 |
October 28 |
1027 |
October 29 |
1029 |
October 30 |
1030 |
October 31 |
1032 |
November 1 |
1033 |
November 2 |
1034 |
Data
source: W6ELProp |
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Date |
FP Sunset Time (UTC) |
October 23 |
2039 |
October 24 |
2038 |
October 25 |
2036 |
October 26 |
2034 |
October 27 |
2033 |
October 28 |
2031 |
October 29 |
2030 |
October 30 |
2028 |
October 31 |
2026 |
November 1 |
2025 |
November 2 |
2024 |
Data
source: W6ELProp |
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Date |
FP Sunrise Time (Local) |
October 23 |
0720 |
October 24 |
0721 |
October 25 |
0723 |
October 26 |
0724 |
October 27 |
0726 |
October 28 |
0727 |
October 29 |
0729 |
October 30 |
0730 |
October 31 |
0732 |
November 1 |
0733 |
November 2 |
0734 |
Data
source: W6ELProp |
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Date |
FP Sunset Time (Local) |
October 23 |
1739 |
October 24 |
1738 |
October 25 |
1736 |
October 26 |
1734 |
October 27 |
1733 |
October 28 |
1731 |
October 29 |
1730 |
October 30 |
1728 |
October 31 |
1726 |
November 1 |
1725 |
November 2 |
1724 |
Data
source: W6ELProp |
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How Sunrise / Sunset time is defined |
Sunrise / Sunset time is typically defined as one of following three
conditions:
- Civil sunrise/sunset corresponds to the center of the Sun
being 6 degrees below the horizon
- Nautical sunrise/sunset corresponds to the center of the Sun
being 12 degrees below the horizon
- Astronomical sunrise/sunset corresponds to the center of the
Sun being 18 degrees below the horizon.
- The foregoing three conditions were likely established for the
'ability to see' or monitor certain atmospheric conditions, not
Ionospheric issues. The W6ELProp
program doesn't use any of the three conditions since it simply defines
sunrise/sunset as when the center of the Sun is on the horizon –
not 6, 12, or 18 degrees below the horizon.
The problem with defining sunrise and sunset for Ionospheric purposes
is that it means different things for the different regions of the
Ionosphere. For the higher HF bands, illumination of the F region is
what's important (for MUF issues). For the lower HF bands, illumination
of the D region is what's important (for absorption issues). Since the D
region and the F region are at different heights, the times when the Sun
illuminates them will be different. Couple this with the fact that the
ionosphere is quite dynamic and thus the processes vary on a day-to-day
basis. So trying to pin this down to the exact minute is, going to the
extreme.
The bottom line on sunrise and sunset time is simple -- it's a window
of low-band opportunity, and one needs to know the general area of this window
to be amongst the Deserving.
Drawing on empirical wisdom to substantiate the
importance of sunrise and sunset in the grand scheme of DX'ing..... Red Eyed Louie was once heard to say,
"One must give full consideration to the overall factors and the
interplay of the various forces. But if you are in the know, you will
recognize it."
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Last modified
July 16, 2004
by Paul B. Peters,
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Copyright © 2000 -2004 Paul B. Peters, VE7AVV. All rights reserved.
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