Tuesday, August 27, 2013

Solar Angle or Length of Day?

In response to my last post about diminishing solar insolation, readers Gary and Mike suggested that the rapid late summer decline in available solar radiation has more to do with the decreasing angle of the sun above the horizon than the decreasing length of day.  It is an interesting question as to which of these effects is more significant in reducing the available solar energy as the season advances.  Is the pronounced loss of solar insolation at this time of year mainly caused by the sun being lower in the sky and thus "weaker", or is the shortening of the day mainly responsible?

The first thing to notice is that the solar angle is clearly the only factor at play in the high Arctic (say above 80 °N), where the first sunset of autumn is only now approaching.  With the sun continuously above the horizon until now, length of day is not an issue; the rapid decline in solar insolation is ALL caused by lower sun angle.  This fact also suggests that solar angle may be the most significant part of the equation at other less extreme northern latitudes, such as Fairbanks.

To take a closer look at the problem, I used the theoretical minute-by-minute solar insolation calculation to determine the loss of incoming radiation caused only by the shortening of the day.  This is simply the amount of radiation received on June 21 during sunlight hours that no longer exist on subsequent dates.  For example, on August 1 in Fairbanks the length of day is over 3 hours shorter than on June 21, so we can say that the shortening of the day caused the loss of the radiation in those 3+ hours.  The chart below shows the accumulation of this loss with the red markers.  The green markers show the total percentage loss of insolation since the solstice (note the 63% value on September 22 matches the results in my prior post).  Finally, the blue markers show the difference, which we can call the loss from decreasing solar angle.



Based on these results, the answer is clear: decreasing solar elevation angle is a much bigger contributor to the total late summer decline in solar insolation.  The shortening of the day becomes a significant factor as the autumn advances, but the elevation angle is the dominant player.  Kudos to Gary and Mike for intuitively recognizing this, and for helping to clarify my thinking.

7 comments:

  1. Here are some numbers that I picked out of a solar energy spreadsheet that I have. Let's use Houston, TX (my hometown), and Fairbanks, AK. I picked a date for Houston, November 1st, and looked for the dates in Fairbanks when the values matched.

    On 11/1, in Houston, the max solar elevation is 45.6 degrees, the length of a day is 11:00, and the theoretical total solar energy is 286 W / sq. m. Now let's find the analogs for Fairbanks.

    Fairbanks has a max solar elevation of 45.6 degrees on May 21st (the same as Houston on 11/1). On that date, the day length is 19:24 and the solar energy is 432 W / sq. m.

    Fairbanks has a day length of 11:00 on October 3rd (the same as Houston on 11/1) . On that date, the max solar elevation is 21.0 degrees and the solar energy is 137 W / sq. m.

    Fairbanks has a theoretical solar energy value of 286 W / sq. m on August 29th (the same as Houston on 11/1) . On that date, the max solar elevation is 34.3 degrees and the day length is 14:55.

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  3. Richard without your fine analysis we'd still be speculating...intuition aside. Thanks for the time spent.

    This all harkens back to Spring snow melting in Interior Alaska. At some point in about March to early April, and at some undetermined value of insolation, we see the first signs of snow melting from solar heating. Entrained relatively dark dust and debris speeds the process. Finally the Sun provides a visible effect on our environment.

    PS: I can use the word better now I that understand what it means and how it's measured thanks to this enlightening Blog: http://en.wikipedia.org/wiki/Insolation

    Gary

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  4. Another aspect of calculating daily instantaneous or cumulative insolation is that the elevation and azimuth of the sun changes throughout the photoperiod. And any daily effect on insolation caused by sun elevation will vary with the latitude of the location.

    Calculating this can get complicated and involves more math than I care to pack around.

    Gary

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  5. I did a post that gets at this question:

    http://ak-wx.blogspot.com/2012/01/how-much-solar-heating-is-there-in.html

    This is the daily integrated solar heating. Note the much steeper decline during August at 65N vs. 40N. At 65N, this plot suggests almost a 30% decline in heating in August alone.

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