Even in the cloudiest days, the valley bottoms tend to have some openings, suggesting that a mobile eclipse watcher would have a good chance of finding a place to watch the Sun, particularly as it is relatively high in the sky (60°). A detailed map of each state along the path of annularity can be found below. The centreline is not representative of the whole of the track, however, as Figure 11 shows that the cloud cover increases much more quickly over the south side of the path.
With the Coast Range on one side and the Cascade Range on the other, the valley has a well-deserved reputation for a dry and sunny environment. The annular eclipse of 14 October, 2023, is the second of three eclipses that cross the United States in the eight years between 2017 and 2024. runs in a continuous loop.This graphic, provided by Dr. Andrew Sinclair, shows the The area would be suitable for those wishing to be at the limit with its spectacular display of Baily’s beads.As the eclipse track passes the Warner Mountains and crosses into Nevada, it enters the Great Basin, a large elevated plateau that covers most of Nevada, half of Utah, and parts of the surrounding states. Small rises in the terrain are matched by small upward bumps in cloudiness, but the High Desert offers the best eclipse-watching prospects in Oregon. The greatest difficulty might be in finding an opening big enough to be able to see a sun that is only 25 degrees high.Over the Great Basin, it is the Sierra Nevada Mountains along the California border that are the biggest wave generators so Nevada is more affected than Utah because of its proximity to the Sierra. It is only when the track reaches the Yucatan Peninsula and beyond that cloudy skies become a significant threat.The high Sun of the tropics is a potent force in warming the ground and initiating the growth of convective clouds. In 19 years of satellite coverage, an observer at Neiva would have been able to see the eclipse with no or a small amount of movement on 13 occasions, four of which would be through thin cirrus. In October, all cloudiness comes from convective buildups, a process that is very sensitive to underlying temperatures.
In 20 years of satellite imagery for eclipse day, Panama enjoyed only one where eclipse watching would have been easy and four where a lucky location could have viewed the event.t is easy to become overly pessimistic about eclipse-viewing prospects when looking at the satellite cloud-cover maps, but, especially in higher cloud locations, the satellite algorithms seem too pessimistic.
These ranges stand only about 1000 m above the surrounding plateau.As the shadow path approaches the Texas border and moves onto the Llano Estacado, October cloud amounts begin to increase. Toward the end of the track, with the Sun less than 10° above the horizon, the eclipse track moves onto the higher plateau of Northeastern Brazil where the seasons are reversed: October is the driest month of the year, and much of the cloudiness melts away, leaving favourable weather prospects as the eclipse sinks onto the western horizon.The eclipse path through the United States begins and ends in modestly cloudy climates, but the midriff welcomes skies with generous sunshine (Figure 3)The lunar shadow comes arrives at the Oregon beaches in familiar country, atop many of the communities that greeted the arrival of the 2017 total eclipse.
A similar pattern is evident in the cloud map, though it takes some effort to fit the cloud pattern to the rise and fall of the terrain. A higher quality version of this global plot can be Over the Yucatan, where the influence of the Atlantic and Pacific anticyclones still have a little currency, the convective clouds are primarily small and easily dissipated.
Most important is their elevations, ranging from 1100 m in the northwest to around 600 m in the southeast, a level that impedes the influx of low-level moisture from the Gulf of Mexico into the region.
It’s a scrubby landscape with wide, open skies and, because it’s a tourist attraction, passable roads and some facilities.
From there, the up-and-down high plains of Nevada’s Great Basin lead the shadow past Four Corners to Texas and the low-lying Gulf Plains before it exits onto the Gulf of Mexico. The lightning strike map of Figure 12 shows that storms are mostly unknown through Oregon, California, and much of Nevada during the month. East of the Andes, over the lowland jungles of the Amazon Basin, cloud cover is high but relatively even, as there is little topography to break up the landscape.Most of the cloud cover in Colombia is convectively generated, but the cloud buildups are early risers, not waiting until the heat of the afternoon to blossom, though they do grow larger toward the latter part of the day.
Be warned, however, that winter starts early at high altitudes, and Crater Lake records an average of 1.9 inches (46 mm) of snow in October (Table 1).For those who want to be first in line for the shadow, the coast of Oregon offers a visitor-friendly environment with plenty of accommodation—and familiarity with eclipses from the 2017 experience. October is beginning the transition to winter and these systems are becoming more common as cold weather approaches.The availability of moisture on the Gulf Plain and the lower parts of the Edwards Plateau has a significant impact on the prospects for eclipse day. Humans place their cities in the bottom of valleys and so sunshine measurements within mountains will reflect the best of conditions.As the eclipse track proceeds eastward, cloud cover grows, from around 75% to 90% as the shadow path moves onto the Brazilian Highlands. Some evidence of this comes from the sunshine statistics (Table 5) for stations in Central America where even in Panama, the average October day experiences sunshine during 35% of the hours.The South American portion of the eclipse begins in heavy weather and ends in sunshine with modest ups and downs in cloud cover along the way. Almost all of the cloudiness over the sertão comes from small cumulus clouds that would likely succumb to the oncoming lunar shadow.Measurements from stations along the track confirm the pattern of cloudiness portrayed by the satellite images.
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