Showing posts with label solar. Show all posts
Showing posts with label solar. Show all posts

Wednesday, June 1, 2022

Sucker Clouds at Sun Baked Observatory


Sucker Clouds at Sun Baked Observatory

When the temperatures rose to over 90-degrees F. in the shade (averaging 120-degrees in direct sunlight), water vapor evaporated and the sun made an appearance in the morning of Thursday, June 2, 2022 - rain momentarily stopped, then sucker holes in the clouds began to appear. How long this will last in unclear as the weather reports rain for the rest of the day.

Parts are slated for ordering to increase the resolution and capacity of Sun Baked Observatory. Improvements are being made to the mounting, guiding, and tracking system. Solar prominences along the sun's limb are being tuned to spectral wavelengths and numerous tests are being performed.

Tuesday, May 31, 2022

Sun Baked Observatory Shroud


Sun Baked Observatory Shroud for Successful Solar Imaging
Imaging the sun with a mobile phone camera function is possible, however the touchscreen can be very problematic. For example, iPhone has a highly reflective screen that reflects so many images in bright sunlight, the photo image on the screen becomes completely lost in the reflective glare.

One simple solution is to make a hood of black material, with plenty of air circulation ventilation. An anti-reflective screen cover may also help. As a third option, go to settings and change the phone screen brightness to maximum.

Saturday, May 28, 2022

Sun Baked Observatory Directory


Sun Baked Observatory Directory

and sun observatories leading up to Sun Baked Observatory

Trials & Tribulations Acuter Maksy 60 at Sun Baked Observatory
https://otisastro.blogspot.com/2022/05/trials-tribulations-acuter-maksy-60-at.html

Sun Baked Observatory Report
https://otisastro.blogspot.com/2022/05/sun-baked-observatory-report.html

Sun Baked Observatory Explores Venus Atmosphere During Solar Transit
https://otisastro.blogspot.com/2022/05/sun-baked-observatory-explores-venus.html

History of Solar Telescopes
https://otisastro.blogspot.com/2022/05/history-of-solar-telescopes.html

SunBaked Observatory
https://otisastro.blogspot.com/2022/05/sun-baked-observatory.html

Acuter Maksy 60 Sun Observatory
https://otisastro.blogspot.com/2022/05/acuter-maksy-60-sun-observatory.html

Sun Telescope
https://otisastro.blogspot.com/2022/05/sun-telescope.html

New Solar Observatory with the Celestron Nexstar 6-inch SE
https://otisastro.blogspot.com/2022/04/new-solar-observatory-with-celestron.html

Log - Solar Telescope
https://otisastro.blogspot.com/2022/05/log-wednesday-may-18-2022.html

Acuter Optics Telescope Arrival - Solar Filter
https://otisastro.blogspot.com/2022/05/acuter-optics-telescope-arrival.html

Solar Eclipse June 21 2020 Taiwan
https://otisastro.blogspot.com/2020/06/images-will-appear-here.html

Venus Transit
https://otisastro.blogspot.com/2020/06/my-observatory.html

High Resolution Solar Observatory
https://otisastro.blogspot.com/2022/04/log-update-celestron-nexstar-6se.html

New Solar Observatory with the Celestron Nexstar 6-inch SE
https://otisastro.blogspot.com/2022/04/new-solar-observatory-with-celestron.html

Log Update Celestron Nexstar 6SE Thursday April 21 2022
https://otisastro.blogspot.com/2022/04/log-update-celestron-nexstar-6se.html

Celestron Nexstar 6SE Log Thursday April 7 2022 - Solar Observatory
https://otisastro.blogspot.com/2022/04/celestron-nexstar-6se-log-thursday.html

Astro Log for Monday April 11 2022
https://otisastro.blogspot.com/2022/04/astro-log-for-monday-april-11-2022.html

Monster Astro Projects - Observing the Sun
https://otisastro.blogspot.com/2021/11/monster-astro-projects.html

My Observatory Summary

Trials & Tribulations Acuter Maksy 60 at Sun Baked Observatory



Above: Attempting high magnification at the Sun's limb produced this unusual appearance - the system needs additional tuning to clearly show sunspots and solar flares and edge prominences.

Exposed with the primary solar filter but no fine tuning engagement of H-Alpha filtering.

Left: at 20mm EP projection and hand holding the iPhone camera, the solar disk was overexposed and getting the iPhone to compensate was insufficient. However, overexposure has advantages and some prominence-appearing minute detail is beginning to appear at the solaredge as well as the graduations towards the photosphere.

Trials & Tribulations of the Acuter Maksy 60 at Sun Baked Observatory
The Acuter Maksy 60 is being tuned for solar work. A number of fixes are needed before this telescope will be fully up and running.

Here's a List of Numerous Anomalies Encountered on Sunday May 29 2022.

Small Stock Tripod Insufficient to Hold Weight
The small tripod mount is insufficient to hold the telescope and the weight of the iPhone.

Small Stock Tripod Cannot Reach Elevation
The small stock tripod must be rotated to a small gap opening at the top to get it to reach a higher elevation, otherwise it bumps into the mount which is very limited. It's inconvenient to stop and move the entire mount and telescope for a position that works better.

Small Stock Tripod Insufficient to Make Fine Motions
The small tripod mount is incapable of making the fine motions needed for adjustments to image positioning

Small Tripod does not fit the Observatory Platform
The small tripod did not fully fit the observatory platform

Stock Phone Mount Failure
The stock iPhone mount failed - mount number one with the stock bands was not fully adjustable and the phone camera would not stay over the eyepiece at the proper position

Phone Mount 2 Failed
The 2nd iPhone mount failed - it pressed on the side of the iPhone against the function buttons and locked p the phone

Phone Mount 3 Failed
The 3rd iPhone mount failed, the lock holding the phone was not able to have fine tuning.

Phone Mount 4 Failed
The 4th phone mount failed, it was too heavy.

Sun Blocked by Roof
Just as the project was getting started, the sun moved into a position blocked by the roof.

Clouds & Haze Obliterates Features
The sun features were relatively void due to viewing the sun through the clouds and haze.

iPhone Touchscreen Failure
The iPhone continued to fail as any touch to the screen activated some unwanted feature.

iPhone Screen Not Visible
The iPhone screen was invisible in the bright sun - a shield was fabricated but it too had too many reflections to see anything.

Two iPhones both Fail
Two different iPhones both had the same problems.

iPhone Goes into Undesired Modes
Just setting on the table, the iPhone goes into undesired modes not conducive to astro imaging. Anything near the screen or touching it randomly is a problem.

Observatory Platform Needs Moving
The observatory platform needs to be completed in construction and moved to an ideal location.

Monday, May 23, 2022

Sun Baked Observatory Explores Venus Atmosphere During Solar Transit

 
Sun Baked Observatory Explores Venus Atmosphere During Solar Transit

We are constantly developing new ways to process and extract data from raw solar imaging. Much of these efforts are experimental and subjective. This time we've enhanced the atmosphere thickness surrounding Venus during a solar transit when Venus was passing in front of the Sun, and looked for Venusian atmospheric detail across the planet.

Topmost Image: This is the final step 4 in the processing cycle. Here we see Venus moving across the face of the sun, approaching the solar limb. The Sun and Venus final result show the appearance of detail in the atmosphere of the planet and a surrounding atmosphere of varying thickness outwards from Venus. The color shows the differentials.

Immediately Above: Step 2 in image processing will determine if any data is present in the raw image as related to the planet and the surrounding region of atmosphere, and if it warrants continued processing.

Left: This is step 3 in the process after
step 2 determines the presence of imagery on Venus and adjacent features, suggesting a surrounding band of thick atmosphere that sunlight is filtering through. The changing solar plane also shows detail closer to the Sun's limb as it receives color encoding to specify the intensity levels of objects discerned. This is also a first level step in reducing the luminosity differential between the Sun and Venus.

At left: Step one in the solar-venus process is to acquire a raw image of Venus traveling across the face of the extremely bright sun. At these great and vast luminosity differences, Venus looks like a black featureless disk, i.e. until processing can view the underlying sheath of light differentials. This image is first processed to reduce the effects of Venus' motion and increase the clarity and sharpness of underlying features.

Sunday, May 22, 2022

History of Solar Telescopes

Venus Transit, ETX-60AT June 6, 2012

History of Solar Telescopes at Otis Astro Imaging

The history of solar telescopes began in 1965 and has continued ever since. Otis Astro Imaging now has these telescopes inside solar observatories doing their work and studies. 

Above: The first solar telescope is a 4.25-inch f/11 reflector from Edmund Co. which is fitted with a purchased accessory glass solar filter, possibly purchased from the former Kenneth Novak and Company. Numerous photos are taken of sunspots and a solar eclipse.

Left: the 2nd solar telescope is a low cost bare bones Celestron 2.99-inch FirstScope f/3.95 Newtonian reflector on a tiny Dob mount - The telescope is fast to setup and lightweight to carry around and transport. It has a focal length of 300mm (12-inches). It was purchased at a toy store in Beijing, China. For solar use, the telescope needs an accessory solar filter film mounted over the front of the telescope tube for best results (sold separately). The grab n go portability and no setup time makes this telescope a first choice for ease of use. General land & Moon images are taken by holding the mobile phone over the eyepiece for eyepiece projection and selecting the best result.

Left: The third sun telescope is the Meade f/5.6 ETX-60AT Refractor is used for solar transits and for studying sunspots. One special study captured the disk of Venus in front of the sun during the June transit and is examining the atmosphere fringes out from the planetary disk and any Venusian surface features.

The 60mm telescope is a precision achromatic refractor on a battery powered GOTO mount. The telescope has very high resolution and is a very good performer. The telescope has a flip mirror, with positions for the eyepiece or straight-through for astro imaging.


Left: 4.5-inch f/4 Orion Starblast is German equatorially mounted and outfitted with an extra accessory electronic sidereal drive and a Chinese solar filter made with Baader solar film. The filter is shared with a second Orion Starblast on a Dob mount.

The second telescope is a Celestron 2.99-inch reflector on a Dobsonian mount that uses solar projection in conjunction with a high concentration of air pollution, in Beijing China. Images were published at the Parallax Forum by Humanoido.


Left: The fifth telescope is the Orion StarBlast 4.5-inch f/4 RFT reflector with a grab and go Dob mount. This telescope shares an identical solar filter with the first equatorial mounted Orion Starblast telescope.

The telescopes have different purposes - one is more ideal for the static observatory and the other is perfect for a portable observatory with the grab and go telescope.


Left: Transit of Venus June 6, 2012 through the 1.6-inch Meade ETX-60AT f/5.6 achromatic refractor.

The third telescope is a Meade ETX60AT (2.6-inch) f/5.8 achromatic refractor used to observe the transit of Venus from a skyscraper rooftop.
https://humanoidolabs.blogspot.com/2012/06/venus-transit-2012.html
A solar sunspot study was made in full color on the previous day of June 5th, 2012 at 4:43:48 pm local time, using ISO125 at 1/400 F5.6 to identify the position of solar spots, test the imaging results, obtain satisfactory full disk image size and resolution, position enlarged disc views, and lock down the setup and imaging procedures. (see June 5th
photo). 

Left: June 6th sunspots photo'd with the Meade ETX-60AT achromatic refractor, during the transit. Approximately nine sunspot groupings are seen. All photos by Otis.

The fourth and fifth telescopes are Orion StarBlast 4.5-inch f/4 with a driven equatorial mount and a grab and go Dob mount. These share a solar filter obtained from China.

Telescope six is a Celestron Nexstar 6SE f/10 on a goto mount that fits the Celestron solar filter.

The newest addition is telescope seven, the famous Acuter Maksutov-Cassegrain Catadioptric 60mm (2.4-inch) f/12.5 with its own solar filter. The solar filter is an extra purchase.

Seen at left, the filter form fits tight onto the front of the Acuter 60mm Maksutov-Cassegrain telescope's OTA. The filter assembly contains a safe projection sun finder molded into the carrier and offset to the side of the filter.

This system is very convenient to carry around (the OTA weighs only one pound) and it has a setup time of only a few minutes. It can compete with finding and utilizing the holes in the clouds to quickly capture views of the sun and sunspots within their 20-minute openings. The setup is ideal for transits and solar eclipses. Others have used the telescope for attaching H-Alpha filters for viewing of the chromosphere, solar prominences etc.

Solar Telescopes
1) Edmund 4.25-inch f/11 reflector
2) Celestron 2.99-inch f/3.95 FirstScope on a tiny Dob mount
3) Meade f/5.6 ETX-60AT Achromatic Refractor
4) 4.5-inch f/4 Orion Starblast Equatorially Mounted with Drive
5) 4.5-inch f/4 Orion Starblast Dob Mounted
6) Celestron Nexstar 6SE f/10 GOTO Mounted
7) Acuter Maksutov-Cassegrain Catadioptric 60mm (2.4-inch) f/12.5

Wednesday, May 18, 2022

Log Wednesday May 18 2022


Otis AstroImaging Log Wednesday May 18 2022

Weather
After I bought the new sun telescope, the local weatherman announced the return of the Monsoon season (rainy season) which is highly unusual for this time of year. I can expect another month of rain every day. This is what happens when you buy a telescope.

Solar Telescope
The Solar Telescope is prepared, filterized, and ready to go when the sky clears. Several times in the late afternoon, the sun briefly appears through haze and in between openings in the clouds. The opening are short lived and the direction of the evening sun is on the opposite side of the observatory - blocked by a tall skyscraper. The roof, thousands of feet high, is a less safe option at this time as high winds often accompany the Monsoon. The higher you go, the stronger the wind. At ground level, there is no wind, but at the upper atmosphere level the clouds can move 1,000 mph. When the cycle of weather rotates, it will flip flop to some brief cloud openings in the morning sky when the sun is properly positioned for solar study.

Observatory Platform
The Observatory Platform needs only 3 more empty water bottles and construction can resume. It takes a total of 40 bottles to complete the backing spacer. Each water bottle base can handle up to 1,000 PSI. The add-on backing is required because the outdoor steel rail has a raised floor foot that prevents the original platform configuration from butting up against the railing. With the added backing, the platform will reach the railing and have a firm strong area for connection. The platform is now made dual purpose, and will have full functionality both indoors and outdoors depending on long term seasonal environmental conditions.

Earthquakes
When installed outdoors, the observatory platform will be anchored to the steel railing with a backing of 40 extra strong 1,000 PSI empty recycled water bottles with a blanket 40,000 PSI strength. The connection is to withstand a category 5 to 5.5 earthquake force jolt. As earthquakes are frequent and common, there's no telling when the next one will occur. Therefore, the platform may remain firmly anchored on the outside observatory and have a covering in place to resist the weathering for at least a season. Earthquakes are another topic regarding the telescopes and will be handled as a separate challenge.

This Pacific area is active geologically, formed on a complex convergent boundary between the Yangtze Subplate of the Eurasian Plate to the west and north, the Okinawa Plate on the north-east, the Philippine Sea Plate on the east and south, and the Sunda Plate to the southwest. Subduction changes direction at this location. The upper part of the crust is primarily made up of a series of terranes, mostly old island arcs which have been forced together by the collision of the forerunners of the Eurasian Plate and the Philippine Sea Plate, which is moving to the northwest. These have been further uplifted as a result of the detachment of a portion of the Eurasian Plate as it was subducted beneath remnants of the Philippine Sea Plate, a process which left the crust underneath this Pacific area more buoyant.

Earthquake-Proof Telescope
One of the best ways to handle the outdoor observatory platform earthquake forces on the telescopes will be to bring in the telescopes to a safer prepared haven indoors after a night of use. For this reason, telescopes are kept lightweight on purpose and are relatively easy to move. Earthquakes shake up and down, left and right, and in contorted directions and can last a full minute, more or less. The force of an earthquake can vary during the earthquake and rapid buzzing and vibration is not uncommon. Telescopes which have a higher center of mass are easy and dangerous targets for quakes to topple. The higher the center of mass, the more the moment of inertia will result. Many small earthquakes are happening all the time, many of which are not detected by human body, or, a feeling of motion sickness may result. There are many ways to detect these - one way is observing things in a residence that will appear to slip, slide and fall without reason. 

Ordering is a Three Step Process
Step one is complete. The sun telescope arrived with the purchased solar filter accessory. Step two remains to obtain solar filter number two and a solar telescope interface to a new mount. Step three remains, to order a number of mixed astro parts necessary to complete intricate operations at Sun Baked Observatory.

Contents
Weather
Solar Telescope
Observatory Platform
Earthquakes
Earthquake-Proof Telescope
Ordering is a Three Step Process

Saturday, May 14, 2022

Sun Baked Observatory

The indoor telescope at Sun Baked Observatory currently looks through a pane of optical window glass to protect against harmful solar UV radiation in the Subtropical Zone. Above, a solar tuning test for image scale and other parameters.

Sun Baked Observatory
The first solar telescope, a 60mm Maksutov-Cassegrain Acuter Catadioptric with a Celestron computer driven alt-azimuth mounting (and other test platforms), is up and running at the new Sun Baked Observatory.

The solar filter and solar finderscope accessory arrived and the system is in place and being tuned. The  new Sun Baked Observatory, equipped with a solar-tuned Acuter Maksy 60 telescope, is located in the dangerous particle-hot Subtropical Zone with exceptional seeing conditions. There is no ozone layer in the upper atmosphere which allows dangerous rays to penetrate - and human cellular cancerous degradation protection against harmful high intense UV is important. For this reason, the observatory is currently being run protectively from indoors, looking through optical window glass. Window glass absorbs UV while passing IR. H-

Alpha test filters are available for experimentation and several cameras and camera mounts are also ready for action. Of course, soon after buying the telescope and accessories, the weather turned to rain. In the future, more of the telescope may be operated by remote to limit harmful solar UV rays exposure to astronomers. 

Overall, the tests thus far are highly successful and an image scale to show the entire solar disk is possible along with increasing magnifications to zoom in on sun features. An optical zoom at 68-degree widefield - Baader Mark IV Hyperion 8mm-24mm (8,12,16,20,24) is being tested along with a camera zoom to test the clarity and resolution of results to test a technique of rapidly going from full solar disk to zooming in on sunspots and other features. This rapidity of change afforded by a zoom lens where time is not lost in changing eyepieces, will facilitate observing through holes in clouds (Sucker Holes) that can disappear in 20 minutes or less. The Sun Baked Telescope needs fast reaction time to be ready in an instant.

Baader Mark IV Hyperion Click-Stop 8mm-24mm (8,12,16,20,24)
Acuter Solar Telescope: 750mm (29.5-inch) FL, 60mm (2.4-inch) aperture

08mm - 93.75
12mm - 62.50x
16mm - 46.88x
20mm - 37.50x
24mm - 31.25x

Under prefect seeing, the maximum power per aperture inch is 50x.
2.4" x 50 = 120x. 6.25mm - 120x

Monday, May 9, 2022

Sun Telescope

The current Solar Observatory at HSO is in full operation with two sun telescopes that share a common solar filter. However, the new upgrade sun telescope is ordered and on the way. The solar disk, seen above, typically has these spectacular features that often go unseen without the right equipment, processing and applications. The upgrade to the solar observatory will include a compliment battery (sum total) of four solar telescopes each with their own respective resources and capabilities. Apertures include 2-inches in Maksutov design, two 4.5-inch RFT Newtonian reflectors for coronal work, a six inch Schmidt-Cassegrain for the highest resolution closeups, and a 3.25-inch refractor being groomed for solar work.



Sun Telescope
The new latest and greatest telescope is on the way - the observatory is a busy place - the order was placed today, Monday May 9, 2022, for a complete solar telescope with a special sun filter. The telescope order with accessories will be delivered on May 11 or May 12 directly to the door, COD and after a cool-down process, assembly with installation will begin. I'm fully prepared to receive it and have placed the cash into a separate transfer plastic bag, awaiting the big moment! The transfer will happen with some extreme degree of pre-arranged protective incognito as safety isolation against the Covid virus.

The telescope is quite spectacular having an ultra high precision Maksutov-Cassegrain Catadioptric design. The short tube length and light weight make it extremely easy to mount. In this case, the telescope will have two dedicated mounts for solar work and also will go alongside another telescope with goto software. This mount is rock solid and very steady, and will include a solar rate sidereal digital drive for imaging sunspots in high resolution. Experiments to find solar flares are anticipated using the primary solar filter and additional Hydrogen-Alpha filters. The sun will be studied in various spectroscopic wavelengths each showing different solar features and compositions.

Specifications: 60mm primary lens coated aperture, OTA tube length 8-inches, OTA weight 1 lb, folded high resolution Maksutov Catadioptric design, features added include ampable to 20-inches and 200-inches. Solar capabilities will include TRANSDIGILOG - Transitional Digital & Analog processing, AMPING - Amplification of Telescope Diameter, and TRANSIS - Transitioning Art in Science. The solar telescope includes a primary solar filter and a built in safety sun finder with safety frosted viewing screen. For safety reasons, the OTA comes with no optical finderscope. The composition of the solar filter is said to include constituent highest quality Baader components with a custom size molded to the shape of the telescope. The observatory assembled system will include a comprehensive kit of vast ranging spectroscopic filters for varying recordable solar wavelengths, eyepieces for full frontal solar disk viewing and highly magnified enlargements for close up views, several camera mounts, multiple cameras including two HD cell phones, one with Live View, and one CMOS astro imaging camera. Additionally assembled for the solar observatory are various power processing computers, PC & Apple, including at least one supercomputer and a minicomputer. Specialized solar software for processing the sun's features will be included in the monitoring and analyzing/processing setup.

Stay tuned for the creation of the Solar Atlas - a systematic compendium of solar images showing the changing face of the Sun. The Sun Atlas will be electronic in PDF format and transferred and distributed via the world wide web. We are opening up a solar section to the Astro Imaging website to report on the changing face of the sun and provide a measure of safety and prediction forecast for the protection of anyone within the sun's path.

Thursday, April 21, 2022

Observatory Log Update Celestron Nexstar 6SE Thursday April 21 2022

Observatory Log Update Celestron Nexstar 6SE Thursday April 21 2022
Update for the construction of a new Nexstar Outdoor Observatory using only simple available parts, materials and no tools

WATER BOTTLES
I now have 12 water bottles - one extra today. I don't know the liter capacity of a bottle but it appears I can down one bottle per day. So this is the data rate of expansion of the water bottle quantity per unit time. The greatest use of water is coffee, tea, drink mixes like potato and protein, other than pure water consumption. The number of empty bottles occurring per day will be monitored and increased if possible. If 50 bottles really are needed (the design may vary), that leaves another 38 required. At one per day accumulated, 38 more days are needed, or just under 6 weeks. If the rate can increase to two per day, that will take 19 days to collect the remainder of the bottles needed, just under 3 weeks in half the time.

BUNGEE CORDS
Bungee cords were ordered from two new companies and are not yet delivered to the door. However, one package will be small and small packages are held at the administration office. Since the admin has new workers, the bungees may not be delivered to the door. The Internet shows at least one package being delivered to the admin. Delivery of the first package is expected today and if it does not arrive, phone calls will be made.

Bungee Update 5:00 pm - After the phone call was made to the building administration, two packages were delivered to the door. One package has eight cords all the same size (19-inches). The 2nd package had only 2 cords (37-inches) and (48-inches). The old cord on hand is (57-inches) and appears to have lost some stretch. It can still be used by supplanting one or two 19-inch cords in the stream. I originally wanted five of each, however by connecting various lengths together, the existing cach of cords may be sufficient to fully complete the project.

WRAPPING
A simple method of wrapping and covering the observatory platform is needed to ward off intense solar radiation, pollution, wind, mist, rain, bugs, birds, dust, and the onslaught damp humidity. The platform will be bungee'd to the metal railing. A technique to insert the wrap tarp under the bungees will be needed. It's likely the solution will encompass keeping the wrap intact on the back under the bungee cords and inserting the protective flaps across the top and front.

ORDERS
Work is proceeding on solidifying the orders for the observatory telescope's accessories from a multitude of vendors. Orders are being handled one at a time. Currently the wait is for two orders for bungee cords. When this arrives in two packages, the next frame of order will include the solar observatory.

WEATHER
Weather is highly changeable as usual and has turned from cold, overcast and raining to a clear blue sunny sky with some patches of upper haze, entirely worthy of solar observations. Weather has completed defied the 10-day predictions and completely baffled the meteorologists to the happiness of local astronomers on the island.

HIGH RESOLUTION SOLAR OBSERVATORY
It has become imperative that we soon complete a new solar observatory, given the increasing number of clear sky days. The decision is not yet made in the purchase of a solar filter accessory. The problems are vendors not providing full information and not having access to full information. In lew of buying a fully equipped expensive solar telescope, a decision will be made soon to select an appropriate safe solar filter. The solar observatory is described in other postings and will be at level 1. Observations will be primarily under the classification of astro imaging with targets being the limb, granulation, sunspots, determination of solar flares and storms, transits and occultation of planets and satellites the ISS International Space Station. Additional studies may measure the variable changing size and shape of the sun, and the distances to the Earth. The telescope employed will be the new upgraded Celestron Nexstar 6 SE in potential amping modes for apertures of at least 6, 60 and 600 inches in diameter.

New Solar Observatory with the Celestron Nexstar 6-inch SE

Log Update Celestron Nexstar 6SE Thursday April 21 2022

Celestron Nexstar 6SE Log Thursday April 7 2022 - Solar Observatory

Astro Log for Monday April 11 2022

Monster Astro Projects - Observing the Sun

My Observatory Summary
Taiwan Skyscraper Rooftop Observatory - Venus Transit Across the Sun

StarryNight Solar Eclipse

Friday, April 8, 2022

New Solar Observatory with the Celestron Nexstar 6-inch SE

Current view of sunspots but without any solar flares - log on Saturday, April 9th, 2022. Enhanced to exhibit sunspot groupings and solar disk granulation.

New Solar Observatory with the Celestron Nexstar 6-inch SE

New Solar Observatory Forthcoming
The Celestron new solar filter #94243 EclipSmart $54.95 + $15.02 shipping for 15-day delivery time, is on the order list for the Celestron Nexstar f/10 6-inch SE. Made of a proprietary Mylar film, the filter is ISO 12312-2 compliant for safe solar viewing, blocking 99.999% of intense light across the entire visible spectrum and 100% of harmful ultraviolet (UV) and infrared (IR) radiation; resulting in high-contrast views of the sun in a neutral color. At just 2.6 ounces, the filter will provide the safety required to observe the sun and all phases of solar eclipses without adding significant weight to the front of the OTA. This replaces the smaller solar observatory with the 4.5-inch RFT f/4 telescope at 1.02 arc second resolution. The larger f/10 6-inch aperture of the Celestron Nexstar will pull in sunspots with a resolution up to 0.93 arcsec (Rayleigh); 0.77 arcsec (Dawes). The resolution is compliant with obtaining high res images showing limb darkening, sunspot groupings, and the extent of solar granulation.

Wednesday, November 10, 2021

Monster Astro Projects

New Orion brand telescopes wait as skies begin clearing

Monster Astro Projects & Updates
The largest projects are described as of Wednesday, November 10, 2021

Numerous ongoing projects make use of the telescopes for astro imaging, conservation, weather, and technical studies. Never a moment lost - if the day is clear, the telescopes are pointed to the mountains to study and statistically categorize the ecology to include plants and animals, large insects and terrain. This area is surrounded by mountains, some 100 miles away, and the telescopes provide exceptionally clear magnified views for visual studies and photographic imaging.

If the night is mostly clear but with sections that may have upper atmosphere haze, or smog, fog, air pollution, heavy humidity, or breaks in the clouds, various inventions are deployed to penetrate the hood to resume astronomical observations.

Main divisions include:
* Singularity Observatory
* Solar Observatory
* Astro Imaging Laboratory
      Equipment, telescopes, accessories purchases
* Conservation
      Forestry study of mountains, plants, animals, birds and resources for
      conservation
* Cartography
      Moon mapping & atlas creation for lunar colonists
* Atmospheric Studies
      Invented methods to penetrate clouds, haze, air pollution, water vapor and haze

Main Sections
* Outdoor Pacific Ocean Astronomy
* Indoor Astronomy
* Armchair Astronomy

Perfect Weather & Clear Skies
The month of November is going exceptionally well. The weather has cooled to the perfect temperature of around 70 degrees and the skies are mostly clear and transparent, providing outstanding views of the mountains for conservation studies and the sky for planetary observations and weather studies. Mother nature has given five months of clear nights after two years of rain and overcast conditions.

Accessories, Inventions
This year has see the purchase of accessories and inventions to penetrate clouds, haze, air pollution, water vapor and haze. 

Telescope Trends
The trend of telescopes: at age 20, the goal was to make the largest telescopes possible. The progression went from 4.25" to 8 and then 12.5. At age 30s, weightlifting helped with strength to build and hoist the world's largest amateur telescope with a plate glass objective at the time - 40 inches in diameter. This was followed by two 50-inch telescopes around age 40s. At age 50s, the telescopes progressed into new inventions - giant power telescopes and then super large space telescopes using recycled nasa parts in space worth trillions of dollars. By age 60s, methods were invented to amplify the power of smaller telescopes into 925 and 1,400 inches aperture. By age 70, the telescope continued to shrink so they could become more manageable, easier to carry and set up.

Digital eVscope Not for this Region
It was finally discovered that, among other problems, Unistellar eVscopes in this region fail due to the combination of severe light pollution combined with haze that occludes and obstructs swaths of stars preventing the telescope from properly calibrating and plate solving.

Busy Making the Lunar Atlas
With renewed interest in the Moon, new private industry moon landings, scientific lunar outposts in the making, upcoming vacation tours to the Moon and potential off-planet colonization, a lunar atlas is in the works. It uses actual raw and processed lunar imaging from our best and most powerful telescopes at Singularity Observatory.

Observing the Sun
Recent telescope upgrades now include a solar observatory, complete with solar filters, abilities to view and image and count solar sunspots to determine sub periods of min and max, transits, eclipses, specula, and other phenomena. Tests will be made on prominences and the solar corona, and correlations with the aurora borealis and aurora australis.