Fort Worth Astronomical Society
 


FWAS Observing Site

The FWAS observing site is in southwestern Wise county. It's about 45 miles from downtown Ft. Worth, has a large parking area, campground, clubhouse, and a restroom. There are 20 concrete pads with electricity, four larger round concrete pads for big Dobsonians. The club owns four 10 inch Dobsonians and two 12 inch Dobsonians for member's use.

The site is open to all FWAS members at all times. Members are asked to please keep site and clubhouse clean, and latch the gate upon leaving. It's also a good idea to take a look at the forecast and check the Clear Sky Clock, provided below, before you plan any trips.

 

Clear Sky Clock

Below is the Canadian Meteorological Centre's (CMC) Clear Sky Clock for the Observing Site in Wise County. To learn how to read the Clock Click Here. The graphic shows the Cloud Coverage, Sky Transparency and Sky Darkness for a 10 mile radius around the observing site.

How to read the Clear Sky Clock

Summary: Find a blue block in the first row. There probably wont be any clouds in the sky then.

Details: Read the image from left to right. Each column represents a different hour. The first two colored blocks in the columns are the colors from CMC's forecast maps for Fort Worth Astronomical Society Observing Site, for that hour. The two numbers at the bottom of a column is the local time, in 24hr format, of that hour. (Local time for Fort Worth Astronomical Society Observing Site is -6.0 hours from GMT.)

The image above shows one hour resolution. But currently CMCs forecasts only every 3 hours. CMC is planning true hourly resolution for summer 2002. In the meantime, the Clock image above will typically show the same color for each triple of 3 hours.

The line, labeled cloud is visible-light cloud forecast. It forecasts percentage cloud cover. Dark blue is clear. Lighter shades of blue are increasing cloudyness and white is overcast. This forecast may miss low cloud and afternoon thunderstorms. CMC's text page explaining this forecast is here.

The line, labeled tran, is the transparency forecast. Here 'transparency' means just what astronomers mean by the word: the total transparency of the atmosphere from ground to space. It's calculated from the total amount of water vapor in the air. Dark blue means excellent transparency befitting Arizona. Light blue is better than average and pale blue is worse than average. White means that there is at least some broken cloud. Look at the cloud forecast for the same time to see how much cloud there will be.The transparency forecast seems to be somewhat pessimistic. CMC's text page explaining the this forecast is here.

The line labeled darkness is not a weather forecast. It shows when the sky will be dark, assuming no lightpollution and a clear sky. Black is a dark sky. Deep blue shows interference from moonlight. Light blue is full moon. Turquoise is twilight. Yellow is dusk and white is daylight. For those who prefer numbers, the scale is also calibrated. The colors represent the limiting visual magnitude at the zenith. The legend row at the bottom shows the magnitude that each color represents, from mag 6, for a dark sky, to mag -4 for daylight. It is based on Ben Sugarman's Limiting Magnitude calculations page. It takes into account the sun an moon position, moonphase, solar cycle and contains a scattering model of the atmosphere. It doesn't consider light pollution, dust, clouds, snow cover or the observer's visual acuity. So your actual limiting magnitude will often be different.