Waxing Gibbous Moon, January 10, 2025, at 7:18 PM EST. Note the delicate “C” shape on the upper left-hand edge of the lunar image — rising sun lighting the mountain tops that line Sinus Iridium while lower terrain remains in darkness. Crater Copernicus stands out at center-left, and Crater Tycho stands proudly in the heavily-bombarded lower area of the image. Note the extensive spread of ejecta rays that radiate across Moon’s surface from the relatively recent formation of Tycho. Photo by James Guilford.
It was a clear night so, of course, I had to go outside and take a look. Cold too, at 13℉, so I didn’t stay long! Mars, Jupiter, and Saturn were easy to find, all three shining bright. I was out for a “Moon shot”, though, got a pretty good one. This was made using our Sun shot setup, minus solar filter, of course! Moon was beginning its occultation of the Pleiades which didn’t image well.
The day was clear, as well, and Moon was clear and bright even against the blue daytime sky. So, here is our neighboring world rising through the trees. This is presented second, instead of at the top, because we prefer the nighttime image.
Waxing Gibbous Moon. January 9, 2025, at 4:08 PM EST. Photo by James Guilford.
The complete solar disk as recorded in hydrogen-alpha light. The “worm-shaped” shadows seen in several areas are filaments. The dark spots are, yes, sunspots. And around the rim or limb of the solar disk are seen prominences — geysers of solar plasma riding magnetic field lines before crashing back into the sun. False color applied.
In addition to photographing Earth’s Sun in white light nearly every clear day, we occasionally set up the heavy telescope mount and bring out the new hydrogen-alpha (Ha) telescope for a bit of visual observing and unique imaging. It’s a bit of work since, without an observatory building we usually feel we need to take down and store away the mount after each session, so we don’t do that every day.
On November 8 we had clear skies, good atmospheric conditions, and the inclination to do the Ha setup and were rewarded with splendid views plus our best Sun images yet.
Using a Barlow lens to zoom for a closer view, we see large and small prominences and hints of spicules along Sun’s limb, and several large filaments. The dark spots in the upper left-hand corner of this picture is a group of sunspots at active region 3889.
Across the solar disk were visible large and distinct filaments — prominence loops seen from “above” — as well as sunspots and swirling patterns in the solar atmosphere around them. All around the Sun’s limb could be seen prominences glowing against a background of black space. Some of the prominences, which are fountain-like sprays and loops of magnetically-charged plasma, were quite large.
A major part of producing good images is what happens away from the telescope. Our usual practice is to record video of the telescope view and use software, in the office, to sort through thousands of video image frames, then stack the best few hundred to form a single still image. The still image is then edited to bring out as much detail and tonal range as possible. This process, which is common in astrophotography, produces a sharper image than what might be acquired via any single photographic “snapshot” owing largely to atmospheric turbulence.
Using a Barlow lens to zoom for a closer view, we see large and small prominences and spicules along Sun’s limb. The dark spot just above the center of this picture is a large sunspot at active region 3879.
There’s room for improvement, and we’re seeing excellent progress, but the images shown here are our best yet of Sun in hydrogen-alpha light.
Note: H-a light is that which Sun is producing in its chromosphere — the solar atmospheric layer between the outer corona and the lower photosphere — and is invisible even to protected human vision and white light cameras. Specialized optics are required to block other wavelengths found in white light and allow observation of Ha. When we observe or image in white light, we’re actually viewing features such as sunspots while looking through both the corona and the chromosphere!
Safety Note: It is not safe to look directly at the sun without specialized eye protection for solar viewing, and safe solar filters for telescope, binocular, or camera use. Permanent damage to vision can result from improper viewing of the sun.
The complete solar disk as recorded in hydrogen-alpha light. The “worm-shaped” shadows seen in several areas are filaments. The dark spots are, yes, sunspots. And around the rim or limb of the solar disk are seen prominences — geysers of solar plasma riding magnetic field lines before crashing back into the sun. Image was recorded and presented here in monochrome.
C/2023 A3 (Tsuchinshan-ATLAS) seen against a starry night sky on the night of October 17, 2024.
C/2023 A3 (Tsuchinshan-ATLAS) has faded so very much in just a few days! We wish that we could have seen it early in the week — right after it became an evening object here — but rain and clouds ruined the first nights and, as I just said, that comet is fading *fast* as it retreats toward the outer regions of our Solar System. Comet C/2023 A3 had what seemed to be an extraordinarily long tail and, while we were unable to capture its extent, you can see hints of it leading far beyond its bright nucleus. Visual sightings, for us, were binocular-assisted only and when we could finally see it, C/2023 A3 wasn’t exactly “spectacular”but it was another comet to add to our “life list”.
C/2023 A3 (Tsuchinshan-ATLAS) the night of October 18, 2024, seen above moonlit, autumn-colored trees reflected in still lake waters. Photo by James Guilford.C/2023 A3 (Tsuchinshan-ATLAS) the night of October 18, 2024. Photo by James Guilford.
A panoramic view of the aurora borealis as viewed from rural Medina County, Ohio, as a surge in activity occurred. The display is reflected in the still waters of a small lake. The bright light at the right-hand end above the treeline is light pollution from the city of Medina. Photo by James Guilford.
It began on Tuesday, October 8, when a sunspot called AR3848 flared explosively over the course of several hours. The detonation hurled a large and powerful coronal mass ejection (CME) Earthward from Sun. On Thursday, October 10 the magnetically-charged solar plasma hit Earth’s geomagnetic field and fireworks erupted. According to SpaceWeather.com the aurora borealis was seen as far south as Puerto Rico!
The area in the upper left-hand portion of this photograph is AR3848, the “active region” that produced an enormous solar flare on October 8, 2024. This is a view of Sun in hydrogen-alpha light, which shows the solar coronosphere layer. Photo by James Guilford.
I headed out to a remote county park location, where I have permission to be after dark, and was fortunate enough to be ready when a significant surge in activity occurred — around 10 PM EDT. That peak was amazing with colors, shapes, and movement visible across the entire northern horizon. It was particularly cool to see pillars appearing and disappearing in real time. Light from the aurora reflected upon the still waters of the park’s lake. Adding to the quiet, magical mood, were occasional calls in the darkness from perched birds. A wood duck, out on the lake, piped a sound reminding me of common loons.
During peak activity, looking east, we see intense red crowning a curved green ring, the Northern Lights reflected from the surface of still lake water. Photo by James Guilford.
The auroral surge went on for probably a bit more than half an hour, challenging me to select a spot to photograph. First one area would glow, then one at the other end of the bow-shaped display, pillars of light would appear like searchlights, then fade away. A thrill to witness as light, movement, and delicate colors were visible to the unaided eye. The camera picked up more than my poor eyes could see but I say without reservation this was the grandest aurora I’ve witnessed.
The western end of the coronal arc appeared strongest, as viewed from Medina County, through most of the evening. Here, during the surge, we see typical auroral colors, curtain-like waves of shape, and pillars that look like they reach the ground or might be mistaken for searchlights projecting from the ground. Photo by James Guilford.
All evening there seemed to be more intense activity over the western end of the aurora; that was verified by relatives in northwest Ohio whose photos showed a sky full of color directly overhead.
Although some observers were concerned that moonlight might drown out the aurora, that was not a problem during the peak or as it began to subside. This image shows the waxing Moon, low to the western horizon, with colorful patches of glowing sky nearby. Photo by James Guilford.
While I was at the lake I heard others coming and going from the park, pretty much the entire time I was there. A young couple eventually ventured away from the parking lot and encountered me at my spot around 11:30, seeking what I had found — a dark spot near the water. Their arrival had been delayed by a camera gone bad, and they had gone home to pick up another. Things petered out not long after the peak and, checking NOAA resources, it looked like the auroral ring was retreating back north. The couple had missed the best of the night and I, with frozen fingers and toes, I headed home.
NOAA Space Weather Prediction Center graphic showing the predicted extent of the October 10-11, 2024 aurora borealis. Observers reported seeing portions of the aurora as far south as the Florida Panhandle. According to SpaceWeather.com it was seen as far south as Puerto Rico!
I’ve been shooting Sun images so frequently lately that I’ve neglected the night. While a recent aurora was obscured by clouds (and my sleep schedule) here, and no Perseid meteors spotted (clouds and sleep), Moon put in a nice appearance. Our neighbor in space was very low in our southern sky the night of August 14, which was good and bad. It was good because it can be hard to observe objects high overhead. It was bad because lower to the horizon means more air — and turbulence — between the observer and astronomical objects than if they were overhead. A tripod-mounted telephoto lens and DSLR were used for the capture and a bit of post-processing sharpened things up pretty well.
One of the things I enjoy most when observing Moon is looking along the terminator — the divide between dark and lit areas — at features partly illuminated by, in this case, the rising Sun. Especially noticeable is the arc of light near the upper end of the terminator — the sunlit tops of the Jura Mountains, defining the Bay of Rainbows, off of the grand Sea of Showers or Mare Imbrium.
Sunspots AR3716, AR3713, and AR3712, imaged June 22, 2024, 12:59 UTC, by James Guilford
I continued my practice of daily imaging of the sun for some weeks now. While still deciding precisely how to use and display the images I’m collecting, I’m also trying to standardize how the images are captured and establish a workflow in editing; that is in an effort to give the daily pictures the same overall size and appearance except for details, such as sunspots, where we want to observe changes. It’s not as easy as it may seem, especially when attempting to constantly improve image quality. This ought to become simpler once I have a permanent setup protected day-to-day within an observatory structure.
Sunspots AR3713 and AR3712, the more pronounced of the three large groups, have been interesting to watch as they traversed the visible side of Sun. Today (June 22), braving the morning’s already hot and humid conditions, I went to the extra work of setting up the Vixen VC200L Cassegrain telescope in an effort to achieve high quality images of the two — plus AR3716 — big sunspot groups before they disappear over the western solar limb. Both of the active regions reportedly harbor opposing magnetic energies which could, at any time, reconnect and throw off powerful flares but both have been surprisingly quiet. The next few days will be the last when an outburst from AR3713 or AR3712 might affect Earth.
The Sun, June 22, 2024 at 13:07 UTC from Medina, Ohio USA. Equipment: Canon EOS 7D Mk. 2, Canon EF 400mm 1:5.6 L Lens, 2X Extender, and Baader Film White Light Filter. False Color Applied. Image Credit: James Guilford / Stella-Luna Observatory
I meant well but still wound up posting new solar images to Instagram and Threads instead of here. Today’s image was particularly pleasing, however, so I’ve posted it in all three places!
Today was another day featuring a cloudy morning and sunny afternoon. This time, however, we experienced excellent seeing for a while — just long enough to record today’s solar portrait. We’re so pleased with the “inset” image that we’re featuring it first — it’s cropped directly from the whole-disk picture. Obviously sunspots AR3713 and AR3712 are dominant features; they also reportedly possess magnetic fields with the potential for M-Class flares.
Doing this the “old-fashioned” way, this image was a single exposure manually selected as best of a larger group of shots. The chosen image is edited to produce the best available picture from the data gathered. Today’s excellent seeing made for an unusually good photo. We’re pretty pleased.
Whole-disk image of Earth’s Sun as recorded June 14, 2024. Sunspot active regions are labeled.
An example of how I have been posting solar images on Instagram and Threads. This particular image shows giant sunspot complex AR3664 the day its coronal mass ejection from days earlier struck Earth’s magnetosphere setting off widespread and spectacular auroras.
I have been posting solar images on a near-daily basis for some time. I enjoy recording the images and sharing them with the world and Sun is an especially interesting object right now as we near Solar Maximum. Unfortunately, I am not sure the daily postings look all that great on Instagram where, now, our home page looks like a collection of spotted oranges or maybe suspect egg yolks! What to do?
My current thinking is to post only the most interesting images on Instagram and Threads — days when giant sunspots are present, newsworthy, or (eventually, when I get it working) spectacular coronal images — unusually interesting shots. To keep a public repository of the other images — the routine, daily views — a page on this website might be advised. I think I’ll try it.
So a daily posting here, on a solar imaging page, and special stuff also posted on Insta and Threads. Yeah, that sounds about right. Thanks for listening. — JG
The first DSLR image of the night turned out to be the most spectacular.
It turned out to be a stronger impact than forecast, and the strongest thus far of this solar activity cycle; the geomagnetic storm of May 10 – 11, 2024 produced auroras (Northern and Southern Lights) visible at night from locations nearly pole to pole.
The Responsible Spot: The morning of the aurora, we photographed Sun, capturing this close-up of AR3664, the source of coronal materials that caused the Northern Lights or Aurora storm. It was a most impressive feature and remained intact and spewing powerful flares as it disappeared over Sun’s western limb!
The forecast of possible aurora prompted me to step outside at about 10 PM (EDT), when twilight had faded, to check the skies. At first I saw what I thought might be clouds but knowing auroras can be feeble, I watched. Sure enough, there was movement in those “clouds”.
NOAA Space Weather Prediction Center’s depiction of the expected extent of aurora May 10, 2024.
Glancing overhead I saw what I found hard believe — aurora ray features directly overhead … at 41º latitude, a rare sight, indeed! Rushing back indoors, I pulled together camera, fisheye lens, and tripod and headed back out.
What most people saw with their unaided eyes resembled thin clouds. Watching those “clouds” as they ebbed and flowed, and subtle coloration betrayed their true nature to those who knew what to look for. The auroral streaks pictured here were directly overhead in Medina, Ohio — 41º latitude.
The aurora still presented itself as cloudy streaks with, perhaps, hints of color. Now also armed with my smartphone, I activated its camera and aimed it at the sky. There on the screen, light amplified by the phone’s electronics, glorious, eye-popping colors filled the sky! I’d never before experienced an aurora like it.
First image of the night came from the iPhone 13 camera, revealing the true extent of the ongoing aurora.
Only occasionally, during the time I was out, did the aurora’s color become visible to me; apparently being just below the limits of my, and others’ visual perception. Another local observer noted color was more visible shortly before I stepped outside to check on things — the actual peak of the display must have happened as twilight was ending and before 10 p.m.
During the hour we watched the show in the sky, the event slowly faded, then returned bringing forth another burst of color. The balance of images here are from a Canon EOS 5D Mk. 4 DSLR camera with a Sigma fisheye lens. The DSLR exposures are ISO 400, f/2.8, and 4 to 8 seconds.
I observed and photographed the aurora from shortly after 10:00 until about 11:30 EDT and in that hour or so, the intensity faded and then re-surged before fading away again which was my signal to shut down. I might have stayed out longer but had a commitment for the next day — sleep was needed — so, satisfied I’d seen the phenomenon at its best, I put away the camera gear.
Looking very nearly straight up, these rays appear to be emanating from a position in the east-northeastern sky. The extent of the aurora was impressive, visible well into the Deep South of the United States. The aurora australis was widely visible in the southern hemisphere.
Knowing it would be all over the news, I submitted my most spectacular shot of the night to the local newspaper — a daily that publishes on Saturday but not Sunday. It was too late for the Saturday edition but the editor gave my photo a three-column, Page 1 spot on Monday.
Colors rain down on a quiet residence, perhaps poured out from the Big Dipper seen here in an inverted position. The north star, Polaris, is a tiny dot near the center of this picture. (Note how two stars of the Dipper’s bowl point toward Polaris.) The short horizontal streak to the right of Polaris is a moving airplane’s navigation lights, captured in the several seconds of the camera’s exposure.
Our Sun is still in its peak activity period, by some accounts it won’t hit solar maximum until some time in 2025, so there may be more auroras in our near future but this was one for the history books!
Page 1 of the Medina County Gazette, Monday, May 13, 2024.
Many eclipse watchers were, with unaided eye, able to see the bright pink or red prominence shown here in our heavily-cropped image of the April 8, 2024 eclipsed sun. The prominences appear red because they are composed primarily of hydrogen which, at high temperatures, emits red light. Image rotated to place the prominence at top for aesthetic reasons. Image Credit: James Guilford / Stella-Luna Observatory.
While we very much wanted to view and photograph Sun’s corona during the April 8 total solar eclipse, a blanket of high, thin cloud covered the area blocking faint details. We were, however, able to observe and image the bright inner corona and prominences (“proms”) along the rim of the eclipsed Sun and what a show it was.
Sun is in the active phase of its 11-year cycle and, during totality, prominences were expected and seen in various sizes and at several sites around the rim. The largest was easily spotted with the unaided eye, causing questions from casual observers as it brightly shined at about the six o’clock position of the eclipse ring as viewed from North America. We were delighted with the images of proms that we were able to acquire!
As Moon drifted across Sun during totality it, in turn, covered and exposed different regions of Sun’s limb. To give a fuller impression of prominences seen, we grafted two of our images from totality into one picture; one image was recorded just as totality began, the other as totality was about to end. The resulting picture is not a view one would have had but does correctly illustrate the position and visual size of the proms.
Two images of totality are combined here to illustrate the visual size and placement of promiences exposed during totality of the April 8, 2024 total solar eclipse. The large loop of the prominence near the six o’clock position was easily spotted with the unaided eyes of many, adding to the wonder of their eclipse experience. Image Credit: James Guilford / Stella-Luna Observatory.
Observers in Northeast Ohio were fortunate. Although the morning began with heavy cloud cover, skies cleared and allowed decent viewing of the eclipse in its entirety. Temperature drops were easily felt as bright daylight transitioned to an eerie twilight. As totality began, cheers of awe could be heard from gathered eclipse watchers at a nearby organized event. Automatic street lights illuminated. A robin was heard singing its evening song. Sunset colors lit the horizon about three-quarters of the way around us. In the southwest, beneath the eclipsed Sun, the horizon appeared dark. And then, as bright sunlight returned, first via a brilliant crescent, then by an expanding and warming solar disk, it was over. Those we spoke with were delightedly awestruck having had the experience of a lifetime.
Following are several images of Sun as the eclipse began, during the partial phase, and as it ended. Times are expressed as UTC and were recorded automatically by the camera, set via GPS. Observers in different areas will have seen times that differed from ours and each others due to parallax effects, Moon being much closer to Earth than is Sun.
First Contact: The first noticeable encroachment of Moon over the solar disk is shown here. This image was recorded at 17:58:34 and marks the beginning of the eclipse process. Two areas of sunspots are also noted here. Image Credit: James Guilford / Stella-Luna Observatory.Sunspot AR3628 was about to be covered by the silhouetted Moon as the eclipse progressed from the lower right-hand area of this image toward the upper left. This was imaged at 18:40 UTC. Image Credit: James Guilford / Stella-Luna Observatory.Fourth Contact: By this point most casual, and many serious observers, had packed up satisfied with a wonderful eclipse experience. We kept the camera running, just so that this instant could be recorded — the moment when Moon completed its passage in front of Sun, in this picture at 20:28:35 UTC. Image Credit: James Guilford / Stella-Luna Observatory.
Stella-Luna Observatory 