It's the astronomer's forecast. At a glance, it shows when it will be cloudy or clear for thenext few days. It's a prediction of when Kansas City, KS, will have good weather for astronomical observing.
The data comes from a forecast model developed by Allan Rahill of theCanadian Meteorological Centre. CMC's numerical weather forecasts are unique because they are specifically designed for astronomers.But they have 1180 forecast maps. It can be a chore to find the one map that tells you if you can observe tonight.
So, I (Attilla Danko) wrote a script to generate the images like the one abovewhich summarizes CMC's forecast images just for Kansas City and the surroundings out to about 10 miles.
There are charts for 6189 locations.
Details: Read the image from left to right. Each column represents adifferent hour. The colors of the blocks are the colors from CMC's forecast maps for that hour. The two numbers at the top of a column is the time. A digit 1 on top of a 3 means 13:00 or 1pm. It's local time, in 24hr format.(Local time for Kansas City is -6.0 hours from GMT.)
|Overcast||90% covered||80% covered||70% covered||60% covered||50% covered||40% covered||30% covered||20% covered||10% covered||Clear|
Accuracy averaged over North America for a 30 day period: when the forecast is predicting less than 12 hours into the future,mostly-clear forecasts (cloud<25%) have been right 80% of the time. Mostly-cloudy forecasts (cloud>75%) have beenright 91% of the time. When the forecast is predicting more than 36 hours into the future, the mostly-clear accuracyis 76% and the mostly-cloudy accuracy is 89%.
It's always wise to click on a colored block for the hour you want to observe and see if your location is close to a cloud edge.
CMC's text page explaining this forecast ishere.
|Too cloudy to forecast||Poor||Below Average||Average||Above average||Transparent|
The line, labeled Transparency, forecasts the transparency of the air. Here 'transparency' means just what astronomers meanby the word:the total transparency of the atmosphere from ground to space. It's calculated from the total amount of water vapor in theair. It is somewhat independant of the cloud cover forecast in that there can be isolated clouds in a transparent air mass, and poor transparency can occurwhen there is very little cloud.
Above average transparency is necessary for good observation of low contrast objects like galaxies and nebulae. However, open clustersand planetary nebulae are quite observable in below average transparency. Large globulars and planets can be observed in poortransparency.
A forecast color of white formally means that CMC didn't compute the transparency forecast because the cloud cover was over 30%. So it maybe possible to observe during a white transparency forecast, but the real transparency is usually yucky.This forecast does not consider smoke. So see the separate smoke forecast line on this chart.
CMC's text page explaining the transparency forecast is here.
|Too cloudy to forecast||Bad 1/5||Poor 2/5||Average 3/5||Good 4/5||Excellent 5/5|
Bad seeing can occur during perfectly clear weather. Often good seeing occurs during poor transparency. It's because seeing is not very related to thewater vapor content of the air.
The excellent-to-bad seeing scale is calibrated for instruments in the 11 to 14 inch range. There are some more details in CMC's seeing forecast page.
No computer model forecasts convective heating well, so consider the seeing forecasts for daytimehours to be less accurate. Seeing is forecast for 3-hour blocks, so triples of seeing blocks will show the same color.A white block on the seeing line means that there was too much cloud (>80% cover) to calculate it.
Note also that you may observe worse seeing though your telescope than what a perfect seeing forecast would predict. That is because tube currentsand ground seeing mimic true atmospheric seeing. You may also observe better seeing than predicted here when observingwith an instrument smaller than 11 inches.
This video discusses the difference bettween tube currents and seeing from 24:23 to 34.06: on youtube.
It is based on Ben Sugerman's Limiting Magnitudecalculations page. It takes into account the sun's and moon's position, moon phase, 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 oftenbe different.
A note about CMC's smoke forecast colors:The chart shows different colors than the corresponding maps because the maps use white to mean "no smoke" but the cloud and transparency forecasts use white to mean "opaque sky".I've chosen colorsfor the smoke line on the chart that might better represent the color of a smokey sky -- except for the highest levels which, when forecast, means people should stay indoors.
The data comes from Environment Canada's Canada's Wildfire Smoke Prediction System.
|>45 mph||29 to 45 mph||17 to 28 mph||12 to 16 mph||6 to 11 mph||0 to 5 mph|
|<25%||25% to 30%||30% to 35%||35% to 40%||40% to 45%||45% to 50%||50% to 55%||55% to 60%||60% to 65%||65% to 70%||70% to 75%||75% to 80%||80% to 85%||85% to 90%||90% to 95%||95% to 100%|
Humidity variations can indicate the likelihood of optics and eyepieces dewing.
But dewing is not simply correlated to relative humidity. Dewing tends to happen when the sky is clear, the temperature is dropping and thereisn't much wind. Being on a hilltop or in a small valley can make the difference between no dew and dripping telescopes. Unfortunately, thehumidity forecast does not have the spatial resolution to know about small hills, valleys, or observatory walls. All of which can reduce dewing.
A sudden spike in the humidity forecast, an hour or so after the cloud forecast predicts a sudden transition from cloudy to clear, when there is no wind, means that ground fogwill form.
Also, when the cloud forecast is opaque and the humidity forecast is 95%, rain is likely: a good time to cover the telescopes.
Since there are many different levels in this forecast, with similar looking colors, it's best to activate the"explain colors when you mouse over" to interpret the colors.
|< -40F||-40F to -31F||-30F to -21F||-21F to -12F||-12F to -3F||-3F to 5F||5F to 14F||14F to 23F||23F to 32F||32F to 41F||41F to 50F||50F to 59F||59F to 68F||68F to 77F||77F to 86F||86F to 95F||95F to 104F||104F to 113F||>113F|
Cold temperatures also mean reduced battery capacity, stiffer lubricants, stiffer electrical cables and slower LCD displays.Camera sensors will have reduced noise. But, in general, electronics have a lowest temperature at which they will work.
To see CMC's full map for a particular hour, click on a colored block. The CMC map your browser will loadwill be the map closest to the hour you picked. The time on the CMC map might look odd because it's in GMT, whilethe blocks on the chart are in local time.
It's worth checking a few of the full maps beforecommitting to a long drive out to an observing site.
Or, if you would prefer a simplified thumbnail:
But please don't copy other html or text from this page.
Just keep using it. I intend to keep updating this image for as long as CMC is willing to generate the underlying maps. But there are waysthat you can help:
If you find this clear sky chart, or CMC maps linked by the colored blocks,useful please send Allan Rahill of the CMC an email (and feel free to copy me). Allan needs to show his boss thathis astronomy forecasts are actually being used.
You can also help keep clear sky charts free for everyone by being a sponsor. Please feel free to tell sponsors that they're cool.