Advertisement
Quick Links
ION
Introduction:
Congratulations on your purchase of a DayStar Filters
the following important instructions before using the filter.
Cautions & Warnings:
Solar Observing with a telescope is sensitive to certain risks. Caution and
care of the telescope and filter is advised in assembly, use and dismantling at all
times. Telescope owners must use caution when affixing the filter to the telescope
never to point any telescope at the sun without the solar filter safely installed first.
While observing, owners must take care and caution that all parts of the filter and
telescope assembly are properly affixed and that no pieces have been opened, tampered with or removed. Owners must also use
caution when the telescope is being dismantled for the day to assure solar filters are never removed while the telescope is pointed
at the sun. Responsible owners will be prudent to inform guest or novice observers of the special nature of the telescope
configuration so not to imply that telescopic observing of the sun is safe without proper filtration.
The DayStar Filters
end plates are affixed with Phillips head screws and are designed for owners to remove themselves. These plates allow owners to
configure the filter as best suits the telescope application. Inner, Delrin plastic end plates, are affixed with allen‐headed screws and
should never be removed outside of the DayStar Filters Laboratory. These delrin end plates hold the optical components in under
slight pressure. Should the delrin plates be removed and pressure released, both minor and major damage to the optical
components can occur.
There are no user‐serviceable parts inside the delrin end plates of the ION filter. ION filters are tamper evident and filters
which have had their housings opened will be void of warranty coverage. To reduce the risk of electrical shock, do not disassemble
the ION filter. This device complies with part 15 of the FCC Rules. Operation is subject to the following two conditions: (1) This
device may not cause harmful interference, and (2) this device must accept any interference received, including interference that
may cause undesired operation.
ION Filters
are subject to premature ageing in hot and humid environmental conditions. ION filters are best if stored
inside the provided weatherproof sealed case whenever not in use. Whenever possible, owners should maintain desiccant anti‐
humidity packs inside the case so as to minimize impact from seasonal changes in ambient humidity.
Installation and Application:
ION Filters
application on Dobsonian or Newtonian telescopes. Smaller, Maksutov telescopes will use application methods common to
ION Filters
Refractor telescopes. All
protect the telescope from overheating.
SCT Telescope Configuration:
SCT Telescopes employ a front mounted Energy Rejection Filter (ERF) with an off‐axis opening of
reduced aperture. By reducing the aperture, the focal ratio of your SCT will be increased from the
native F/6 to F/10 to an ~F/30 beam. Because the SCT has a central obstruction from the
secondary, we need to move the opening off‐axis. Now the beam that exits the SCT telescope will
be smooth and parallel when it reaches the rear mounted DayStar
reduction does not change your overall focal length. Your image size will remain the same as before
Filter
ION Filters
will arrive installed with 2 aluminum and 2 Delrin end plates. The outer, aluminum
may be applied on refractor, SCT, or Maksutov reflector telescopes. DayStar does not currently suggest
in any application require both an approximately F/30 light cone and Energy Rejection to
.
ION Filter
Please read
ION Filter
Daystar Filters
. Aperture
Advertisement
Related Manuals for DayStar Filters ION FILTER
Summary of Contents for DayStar Filters ION FILTER
- Page 1 Daystar Filters Filter Introduction: ION Filter Congratulations on your purchase of a DayStar Filters Please read the following important instructions before using the filter. Cautions & Warnings: Solar Observing with a telescope is sensitive to certain risks. Caution and care of the telescope and filter is advised in assembly, use and dismantling at all ...
- Page 2 Filters are 60mm or greater. Please see our website at www.DayStarFilters.com for the correct ERF for your SCT Telescope. ION Filter The DayStar can be affixed to the rear of the SCT telescope with an adapter typical to photo applications from SCT to T‐thread. For those who don't own this part, we stock it as part number: GF2SCTT. It is a small snout with male T‐threads on one end and a female ION Filter "jingly ring" on one end which allows you to orient the DayStar (or camera) on the back of the SCT thread. See our adapters and snouts page for more information about the GF2SCTT http://www.daystarfilters.com/AdapterSnouts.shtml ION Filter The DayStar will thread to the GF2SCTT via female T‐threads on its "sun side" plate. Due to the off axis ERF, light entering the ION will be coming into the filter at 1.9° off the telescope’s central axis, which unless corrected will cause the filter passband to shift off H‐Alpha. Therefore, always use a Wedge plate on the front of an Ion when using an SCT telescope. See part number: Q3GWTF on our adapter plates web page: http://www.daystarfilters.com/AdapterPlates.shtml ION Filter When you order your DayStar , we will ask what telescope it is to be mounted on. If the answer is SCT, then a Wedge plate is supplied at no extra cost ION Filter with the filter order ‐ mounted to your DayStar at our factory. Once the DayStar Filter is attached to the Telescope, the orientation of the filter must be aligned to the orientation of the ERF opening. With light and knob facing up at the 12:00 position, the ERF hole must orient down to the 6:00 position. If in doubt, dial the ERF 360° to find the orientation that provides the best contrast. ION Filter The rear plate on the DayStar ...
- Page 3 Refractor configuration includes energy rejection by means of a front‐mounted colored glass ERF, which blocks all light below 500nm. Some refractor owners opt for Energy Rejection Filter application by means of UV/IR cut filter mounted toward the rear of the telescope instead. This topic will be addressed specifically in higher detail below. ION Filter The Assembly order of the DayStar on a refractor telescope goes: ERF Telescope OTA Diagonal Powermate Barlow (We recommend use of Powermate PMT adapter to thread directly to the ION) Ion Filter, KNOB side towards barlow SCT‐2” or 1.25” (visual back) adapter Eyepiece or camera The UV/IR cut filter Certain refractor telescope owners may choose to employ a UV/IR Cut filter for means of energy rejection INSTEAD of a front mounted colored glass ERF filter. Not all refractor telescopes may use this option. The UV/IR cut filter is a dielectric coated filter that reflects UV and IR light like a mirror. It does not absorb light and therefore is not susceptible to heat gain or expansion like colored glass ERF's are. Applied correctly, the UV/IR cut filter acts similarly to a Herschel Wedge, reflecting much of the spectrum back out of the telescope, while passing a smaller percentage of light. In the case of the UV/IR cut filter, the light which is allowed to pass is the entire visible spectrum. UV/IR Cut filter shown threaded on the end of the 4X Powermate on a DayStar Quantum Filter. Also shown is the 4X powermate with PMT adapter. *IT MUST BE NOTED THAT A UV/IR CUT FILTER IS NOT SUFFICIENT FILTRATION FOR SOLAR VIEWING ALONE. * Because the UV/IR Cut filter acts as a mirror, it is best inserted in the light path prior to any other optical element which might encounter concentrated light. For example, the UV/IR cut filter may be threaded onto the front snout of the forward section of a diagonal mirror. Most diagonals offer filter threading in their front end. If a powermate or barlow encounters concentrated light before the diagonal, then the UV/IR cut filter should be threaded onto the lead end of that element. Unwanted light which hits the UV/IR cut filter is then reflected back out the front of the telescope, arriving at the objective lens at nearly the same unfocused beam as it does coming through the front side. ...
- Page 4 ION Filter Operation ION Filter The was designed for simplicity in operation. Once the ION filter is installed on the telescope, use the following steps: ION Filter 1: Plug in the with the included 12VDC power adapter*. A yellow light will come on. 2: Assure that the knob is in the center‐most detent stop position, as shown in the photo below. 3: Wait the approximately 5‐6 minutes until the filter has reached the correct temperature. The light will turn green. When the light is green, the filter is on band and ready for observing. Tuning: ION Filter The provides the option for a slight variation in wing shift tuning. That means the filter can be tuned to transmit slightly lower or higher than 6562.8Å in wing shift. This allows the user to explore the effects of wing shift on features of the sun; or ION Filter to make minute adjustments of the filter based on special circumstances which might occur. The can be tuned with the knob; up to 0.5Å in each direction, red and blue wing. The dial is calibrated with steps of 0.1Å movement in wing shift. Each time the dial is changed to a different position, the light will change yellow until the adequate time has passed to change the filter temperature and settle through the optical glass. *The Included 12VDC power adapter converts 110‐240VAC to 12VDC. Owners will note that the box includes a variety of various outlet plug style choices for application in most any country worldwide. 12VDC cigarette lighter and alligator clip cords are available.
-
Page 5: Optional Accessories
About Seeing Limitations and Resolution Solar observing seeing conditions vary greatly from nighttime conditions. During the daytime, radiant heating from the sun affects seeing significantly. Characterized by turbulence or shimmering as seen over a hot street, seeing can cause significant impact on quality of solar observations. ‐ Bad seeing is caused by air of different temperatures mixing. This typically happens within the lowest 10 feet of air. It occurs most often over pavement, dark objects, rooftops and sometimes trees. ‐ High cirrus clouds or “scuzz” will cause scattering of sunlight in the high atmosphere which often makes for bad viewing conditions. A classic sign of high cirrus clouds is the inability to achieve focus, or the need to “chase focus”. ‐ A jet‐stream moving overhead can also hurt seeing conditions even on a clear day. DayStar Filters are high power viewing platforms and this high resolution can be susceptible to seeing issues. Solar Observers using high powered, high resolution telescopes and DayStar filters should heed daytime seeing. While many of these conditions are beyond our control, observing in an area with ideal conditions, without pavement in the direction of viewing, and on days with no high cirrus will offer best results. Grass is the best environment for daytime seeing stability. Each observing location offers different behavior for daytime seeing cells at different times of the day, as the air through which one views changes with movement of the sun. Some locations benefit from best seeing in the morning, while many have best seeing in the afternoon. Because most heat variation between air and ground surfaces occurs within the first 10 feet above the ground, often a high observing platform will offer superior seeing. This might include a second story deck which overlooks grass. Eyepiece Selection Daystar Recommends Tele Vue Plossl series eyepieces of 32mm, 40mm and 55mm. Remember that at F/30, a high powered eyepiece can exceed Dawes' limit. Observers will find best results with an eyepiece which is 32mm or greater to avoid this. Eyepieces of higher power will result in a fuzzy disk without the ability to focus well. We have tested a number of eyepieces over the years. Most recently in the spring of 2011, we performed a comprehensive eyepiece comparison between various brand names and eyepiece styles. Naglers, zooms, radians and other "fast" eyepieces typically perform very badly on DayStar applications. Other brands do offer Plossl eyepieces in 32‐50mm and they can give a respectable performance in lieu of a Tele Vue. We have also found some of the very old wide field "Erfle" eyepieces aren't bad for an experienced observer. It should be noted that repeatedly in side‐by‐side tests, we found Tele Vue brand Plossl eyepieces to offer the highest contrast, most even view and widest exit pupil. In Solar Observing, contrast is achieved by control of scattering. Tele Vue Plossls stand out in superior design. Furthermore, the adjustable eye cup offers additional contrast by allowing the user to dark adapt during sunny days. Eyepiece features we found to increase performance include: ‐ "Fully Multicoated" Of those eyepieces which did better than others, those marked "fully multicoated" offered better views from less internal scattering. ‐ Blackened optical edges Tele Vue and other eyepieces which performed better all had blackened edges of their optical elements. This also reduces internal scattering within the eyepiece. Optional Accessories ION filter owners who image may be interested in the “Interference Eliminator” adapter which mounts between the DayStar ION filter and the camera. It eliminates the wavy lines known as “Newton’s Rings,” caused by parallel monochromatic light. 12VDC cigarette lighter and alligator clip style cords are available. ...
Need help?
Do you have a question about the ION FILTER and is the answer not in the manual?
Questions and answers