How to Calculate Hour Angle and Solar Noon: Simplified Guide"

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Discussion Overview

The discussion focuses on calculating the hour angle and solar noon, including the necessary formulas and concepts involved. Participants explore the relationship between solar time, standard time, and the hour angle, as well as the implications of longitude on these calculations.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant seeks to find the hour angle for each day of the year and expresses confusion over the formulas provided by Wikipedia.
  • Another participant suggests a formula for solar time that incorporates standard time, local longitude, and an equation for the equation of time (E).
  • There is a clarification regarding the standard meridian (Lst) being the longitude that corresponds to the local time zone, with examples provided for different US time zones.
  • Some participants discuss the distinction between Lst and Lloc, with Lloc being the actual longitude of the location.
  • A participant mentions the concept of an analemma, which can be observed by photographing the Sun's position at noon over a year.
  • There is a question about the relationship between solar time and solar noon, with a participant seeking clarification on whether they are equivalent.
  • One participant confirms that all equations discussed use degrees rather than radians.

Areas of Agreement / Disagreement

Participants express varying levels of understanding regarding the definitions and calculations of solar time, hour angle, and the relationship between Lst and Lloc. Some points are clarified, but confusion remains about specific terms and their applications.

Contextual Notes

Participants highlight the importance of understanding the differences between standard time and solar time, as well as the need for precise definitions of terms like Lst and Lloc. There is also an acknowledgment that the calculations depend on the correct interpretation of these terms.

dacruick
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Hi. I want to be able to find the hour angle at each day of the year. Wikipedia sent me on a wild goose chase of Julian Day Numbers and some useless formulas that place solar noon at the same time every day. For those who may be used to different terms, hour angle is the amount of time (in degrees) that a position on Earth is away from solar noon. Ideally I would like to be able to find the hour angle, but finding solar noon will also be acceptable as well, as I can find the hour angle from that.

One site suggested that my hour angle is equal to the local sidereal time subtract the right ascension. The problem with this is I don't know how to calculate sidereal time, or right ascension. If anyone could shed some light for me(no pun intended), it would be much appreciated
 
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The Wikipedia article on http://en.wikipedia.org/wiki/Sidereal_time" should help.

Also, this site can calculate it for you based on your location - http://tycho.usno.navy.mil/sidereal.html" .
 
Last edited by a moderator:
Find solar time:

Solar\ Time = Standar\ Time + 4\left(L_{st}-L_{loc}\right)+E

where Lst is the standard meridian for the local time zone, Lloc is the longitude of the location, and E is defined by:

E=229.2\left(0.000075+0.001868\ cosB-0.032077\ sinB-0.014615\ cos2B-0.04089\ sin2B\right)

where B is

B=\left(n-1\right)\frac{360}{365}

and n is the day of the year.

To get hour angle from time, multiply hours from noon times 15 degrees per hour (negative for before noon, positive for after). For example if solar time is 10:30 am, this is 1.5 hours before noon, so the hour angle would be -22.5 degrees.
 
when you say Lst is the standard meridian for the local time zone, what does that mean.
 
It is the longitude that corresponds with your time zone. Examples in the US would be Eastern - 75oW, Central - 90oW, Mountain - 105oW, and Pacific - 120oW.
 
Yeti08 said:
It is the longitude that corresponds with your time zone. Examples in the US would be Eastern - 75oW, Central - 90oW, Mountain - 105oW, and Pacific - 120oW.

I though Lloc was the longitude corresponding to my time zone.
 
If you photograph the position of the Sun at noon (not daylight savings time) every day for a year, you will get an analemma in the sky. See

http://www.1worldglobes.com/analemma.htm

The analemma used to be shown on world globes, usually in the Pacific Ocean, west of South America.

Bob S
 
dacruick said:
I though Lloc was the longitude corresponding to my time zone.
That's your actual longitude for the location. That difference in that equation is to correct for your actual location - while your "normal" time will stay the same while traveling across several degrees of longitude, your solar time will change.
 
I apologize, I don't think I understand what you are saying. I live in Toronto, so my Lloc would be approximately 79 degrees. But you are saying my Lst will be 75 degrees because I'm in the eastern time zone? So my difference will be -4 degrees correct?
 
  • #10
Furthermore, I am doing this to calculate solar time, but I do not know what solar time is. Is the solar time equal to solar noon?
 
  • #11
dacruick said:
I apologize, I don't think I understand what you are saying. I live in Toronto, so my Lloc would be approximately 79 degrees. But you are saying my Lst will be 75 degrees because I'm in the eastern time zone? So my difference will be -4 degrees correct?
Yes, that is correct.

dacruick said:
Furthermore, I am doing this to calculate solar time, but I do not know what solar time is. Is the solar time equal to solar noon?
For solar time, noon corresponds to solar noon. I stated in my first post how to convert solar time to hour angle.
 
  • #12
So my standard time must be measured in degrees as well?
 
  • #13
Yes, I should have said before that all the equations I listed use degrees, not radians.
 

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