The 2024 Solar Eclipse: What’s All the Fuss About?

It’s also cool to hear people around you respond to what they are witnessing. The air temperature becomes noticeably cooler. Scattered low clouds that might have threatened to get in the way mostly disappear, just as they do after sunset.

From Roy Spencer, PhD

April 17th, 2024 by Roy W. Spencer, Ph. D.

I feel fortunate to have witnessed two total solar eclipses in my lifetime. The first was at Center Hill Lake in central Tennessee in 2017, then this year’s (April 8) eclipse from Paducah, Kentucky. Given my age (68), I doubt I will see another.

For those who have not witnessed one, many look at the resulting photos and say, “So what?”. When I look at most of the photos (including the ones I’ve taken) I can tell you that those photos do not fully reflect the visual experience. More on that in a minute.

Having daytime transition into night in a matter of seconds is one part of the experience, with the sounds of nature swiftly changing as birds and frogs suddenly realize, “Night sure came quickly today!”

It’s also cool to hear people around you respond to what they are witnessing. The air temperature becomes noticeably cooler. Scattered low clouds that might have threatened to get in the way mostly disappear, just as they do after sunset.

But why are so many photos of the event… well… underwhelming? After thinking about this over the past week, I believe the answer lies in the extreme range of brightness a solar eclipse produces that cameras (even good ones) have difficulty capturing. This is why individual photos you see will often look different from one another. Depending upon camera exposure settings, you will see different features.

This was made very apparent to me during this year’s eclipse. Due to terrible eclipse traffic, we had to stop short of our intended destination, and I had only 10 minutes to set up a telescope and two cameras, so some of my advance planning went out the window. I was watching the “diamond” of the diamond ring phase of totality, as the last little bit of direct sunlight disappears behind the moon. At that point, it is (in my opinion) possible with the naked eye to perceive a dynamic range greater than any other scene in nature: from direct sunlight of the tiny “diamond” to the adjacent night sky with stars. I took the following photo with a Canon 6D MkII camera with 560 mm of stacked Canon lenses, which (barely) shows this extreme range of brightness.

In order to pull out the faint Earthshine on the moon’s dark side in this photo, and the stars to the left and upper-left, I had to stretch this exposure by quite a lot.

From what I have read (and experienced) the human eye/brain combination can perceive a greater dynamic range of brightness than a camera can. This is why photographers have to fool so much with camera settings to capture what their eyes see. In this case, I perceived the “diamond” of direct sunlight was (of course) blindingly bright, while the sun’s corona extending 2 to 3 solar diameters away from the sun was much less bright (in fact, the solar corona is not even as bright as a full moon). But in this single photo, both the diamond and the corona were basically at the maximum brightness the camera could capture at this exposure setting (0.5 sec, ISO400, f/5.6), even though visually they had very different brightnesses.

Many of the better photos you will find are composites of multiple photos taken over a very wide range of camera settings, which more closely approximate what the eye sees. I found this one that seems closer to what I witnessed (photo by Mark Goodman):

So, if you have never experienced a total solar eclipse, and are underwhelmed by the photos you see, I submit that the actual experience is much more dramatic than the photos indicate.

Here’s some unedited real-time video I took with my Sony A7SII camera mounted on a Skywatcher Esprit ED80 refractor telescope. We were in a Pilot Travel Center parking lot with about a dozen other cars that also didn’t make it o their destinations due to the traffic. I used a solar filter until just before totality, then removed the filter. The camera is on an automatic exposure setting. I’ve done no color grading of the video. Skip ahead to the 3 minute mark to catch the transition to totality:

Crowd-Sourced Experiment During the April 8 Solar Eclipse

A total solar eclipse affords us the opportunity to measure the response of the atmosphere to a known forcing that is very different from the day-to-day hemispheric heating from sunlight superimposed on gradual seasonal changes.

From Watts Up With That?

[This post IS NOT an April Fool’s joke as was the previous]

by Guillermo Gonzalez

Since the 19th century scientists have made meteorological measurements during solar eclipses (https://royalsocietypublishing.org/doi/full/10.1098/rsta.2015.0217). A total solar eclipse affords us the opportunity to measure the response of the atmosphere to a known forcing that is very different from the day-to-day hemispheric heating from sunlight superimposed on gradual seasonal changes. I made my own very small contribution to this topic during the October 24, 1995 solar eclipse in India (https://ui.adsabs.harvard.edu/abs/1997KodOB..13..151G/abstract).

One phenomenon that deserves further study is surface pressure fluctuations produced during a solar eclipse. These have been interpreted as gravity waves. They have been measured at several eclipses, though attempts are not always successful and quantitative results vary.

For examples from the literature, see (https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/JD089iD03p04953?casa_token=-2NygK7STpQAAAAA:TlV1SXPo0Hlj5JdfNIbr7ZpFCgUL8xUpWCDzy0FuGraSbZPOKf2081Gy8bQ4xoSURvOxHbjEig30BcU , https://journals.ametsoc.org/view/journals/atsc/70/3/jas-d-12-091.1.xml?tab_body=abstract-display , https://royalsocietypublishing.org/doi/full/10.1098/rsta.2015.0217 , https://royalsocietypublishing.org/doi/full/10.1098/rsta.2015.0222).

There are a couple reasons published studies of eclipse gravity pressure waves have often had inconclusive results. First, usually only a few instruments have been deployed along the eclipse track. Second, local meteorological changes unrelated to the eclipse (such as a passing front or atmospheric tides) have masked the eclipse waves.

This deficiency can be overcome by deploying many instruments along the path of totality. Sounds like an expensive experiment. It can be done very cheaply with modern technology. Many phones have built-in pressure sensors. They also have built-in GPS sensors, providing accurate locations and times. Phones have multiple additional sensors, making them handy portable scientific data loggers.

My purpose in writing this short post is to encourage as many people as possible to use their phones to gather data during the April 8 solar eclipse with multiple sensors.

The Sensor Logger phone app (https://github.com/tszheichoi/awesome-sensor-logger , https://www.tszheichoi.com/sensorlogger ) can record and store the readings from any combination of your phone’s sensors. I’ve setup a crowd sourced solar eclipse experiment with Sensor Logger. You can join the experiment one of two ways:

1 – Go to https://sensor.tszheichoi.com/app/study/eclipse1 with the browser on your phone and follow the directions to join the experiment. The ID of the experiment is ‘eclipse1’.

2 – Download the Sensor Logger phone app. Then, scan the following QR code with your phone camera and follow the directions:

On April 8 you should be within or near the path of totality to participate in the experiment, but measurements might still be useful even if you’re hundreds of miles from it. Place your phone face up somewhere outside where it will be undisturbed for at least several hours. It should be fully charged at the start of the experiment or plugged into a power source. Start recording data about 3 hours before the predicted time of mid-eclipse at your location and end your recording 4 or 5 hours later. NOTE: your location will be recorded along with light level, magnetometer, sound level, and barometric pressure. If you have the opportunity, also record data 24 hours before and/or after. Your data will be stored by the app on the cloud.

I will collect the data from the cloud and analyze it. Hopefully, I will publish the results in a scientific paper some months later.

Bio: Guillermo Gonzalez is an astronomer who lives in northern Alabama and works for Tellus1 Scientific, LLC. He obtained his Ph.D. in astronomy in 1993 at the University of Washington. He has published over 90 research papers in astronomy and astrophysics journals.

The Next Great Total Solar Eclipse On US Soil Is Now Just About Six Months Away…Monday, April 8th, 2024

From Watts Up With That?

[note from Charles. Anthony and I trekked to Central Oregon to view the 2017 Solar Eclipse, chronicled in this post]

Paul Dorian

This map shows the 20-year (2000-2020) “median cloud fraction” in the month of April at approximately 1:30 pm local time as measured from NASA’s Aqua satellite.  The path of totality on April 8, 2024, is shown with red lines marking the northern and southern limits and a blue line up the center. Based on this climatological cloud cover map, Mexico and southern Texas offer the best prospects for a clear view of totality. Data courtesy: NASA.

Overview

In August of 2017 America went crazy for the first coast-to-coast total solar eclipse on US soil since 1918 and it provided a great opportunity for scientists and all sky watchers. What was referred to as “The Great American Solar Eclipse” took place on August 21st, 2017 when the moon passed between the sun and earth. Total solar eclipses occur somewhere on Earth every year or so, but generally cast their shadows over oceans or remote land masses.  If you missed the 2017 total solar eclipse or it turned out to be cloudy in your particular area then there will be another opportunity in just about six months from now on Monday, April 8th, 2024. This time the Moon’s dark shadow, about 115 miles wide, will cross Mexico, sweep northeast from Texas to Maine, and then darken the Canadian Maritimes. 

Cities inside the totality path for the April 8th, 2024 total solar eclipse (Courtesy GreatAmericanEclipse.com)

Details

The next total solar eclipse visible on US soil will come on Monday, April 8th, 2024. This one will feature a duration of totality up to 4 minutes and 27 seconds which is almost double that of “The Great American Eclipse” of August 21, 2017. It is estimated that the 2017 total solar eclipse was witnessed by around 20 million people from Oregon to South Carolina and the next one is very likely to be viewed by many millions more. The prediction of “many millions more viewers” is quite safe considering the fact that there are 31 million people already living in the totality path which will extend in a southwest-to-northeast fashion from Texas to Maine. 

The solar eclipse of April 8, 2024, will be total in a narrow path from Mexico to the Canadian Maritimes and partial to the northwest and southeast. Yellow curves indicate how much of the Sun is covered by the Moon outside the path of totality. The difference between a total solar eclipse and a partial one is literally the difference between night and day, so get yourself into the path of totality if you can. Courtesy GreatAmericanEclipse.com

In the US, totality will begin on April 8th, 2024 at 1:27 (CDT) in Texas and will end in Maine at 3:35 pm (EDT).  The narrow path of totality—where the Moon covers the Sun completely, causing a total eclipse – runs through Mexico (from SinaloatoCoahuila), the US (from Texasto Maine), and Canada (from OntariotoNewfoundland). And if you happen to live in southern Illinois or southeastern Missouri then you will be lucky enough to be in the “totality zone” for the second time when including the 2017 celestial event. A partial eclipse will be visible across nearly all of North America, and a sliver of western Europe.

This animated GIF shows the Moon’s shadow arcing across the Pacific, then traversing North America, and ending at sunset not far from Spain. The longest duration will be near Torreon, Mexico at 4 minutes and 27 seconds. The inner black circle, the umbra, is where the shadow is complete — a total eclipse of the Sun. The outer shadow circle, the penumbra, shows the extent of the partial eclipse. The partial eclipse will be slight near the outer circle and deep near the path of totality.

During a total solar eclipse, the Moon blocks the Sun’s bright face — the photosphere — briefly revealing our star’s outer atmosphere: the shimmering corona, or “crown.” The corona is always there, but we usually can’t see it because the photosphere is about a million times brighter and drowns it out. When the Moon covers the Sun’s bright face, the corona is definitely the main attraction, and depending on location, the corona will be visible for up to 4 minutes 28 seconds.

These are the times and durations of the eclipse at several points inside the path of the total solar eclipse.

Made of rarefied gas heated to millions of degrees, with its atoms highly ionized (stripped of electrons), the corona gets sculpted into streamers and loops by the Sun’s powerful magnetic field and shines with a light seen nowhere else. Those who have witnessed it say it is hauntingly beautiful and one of the most awesome sights in all of nature. During those moments of totality, it is safe to look directly at the Sun, even through binoculars or a telescope. But whenever any part of the photosphere is uncovered, it is essential to view the Sun through a safe solar filter, that is, one that meets the transmission requirements of the ISO 12312-2 international standard. Such filters are widely available and are not too costly. Looking at the uneclipsed or partially eclipsed Sun through dark sunglasses or any other unapproved filter is a recipe for serious and potentially permanent eye injury. 

Diamond Ring Eclipse By Anthony Watts 8-21-17

At the beginning and end of totality, the thin middle layer of the Sun’s atmosphere, the chromosphere, blazes in an arc of ruby red. The sky darkens to a deep twilight blue, with yellow, orange, and pink sunrise/sunset colors on the horizon in all directions. Bright stars and planets may become visible in the darkened sky and the air temperature will often drop noticeably. The dark sky even tricks nocturnal animals into thinking it’s nighttime and you may hear crickets chirping or see birds returning to their nests.

Remember…when it comes to solar eclipses…99% is definitely not the same as 100%…getting inside the path of totality is critical as this is the only place the corona can be seen.

One final note… after 2024, the next total solar eclipse to be visible from the United States will be in 2044.

Meteorologist Paul Dorian
Arcfield
arcfieldweather.com

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