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DayStar Telescopes and filters

are all HAND MADE. 

• Each instrument is hand

manufactured and assem-

bled one-by-one.  Each is

unique.  Slight variations in

construction that do not

affect performance may

occur.  

• Each instrument is indivudually tested on the Sun.  Sun testing is an

absolute necessity to assure quality performance.  While every precaution is

taken to maintain the ‘like new’ appearance of the telescope, it may

encounter minor cosmetic smudges or abrasions on the mounting foot or

the drawtube during testing. 

• The optical filter stack is assembled by human hands using special optical

couplant that must remain loose for over 10 years.  Occasionally, if dis-

turbed, this couplant can migrate to optical surfaces.  Do not disturb your

optical stack.  If a small amount of couplant is smudged onto your outer

surfaces, it is best not to disturb it. It will not affect performance, like a large

mirror. Larger smears will need to be cleaned by technicians at our factory.

Solar Minimum Notice:

Let us remember that the Sun

has a sunspot minimum and

maximum cycle of about 11

years.  We are currently

experiencing a period of

sunspot minmum that has

lasted surprisingly long.  This

means that the sun may not

have as many exciting things

going on the day that you

view or image, than you may

have seen in photos or in the

past, if during a point of high-

er activity in the past.  

This difference in visible activi-

ty is unrelated to the instru-

ment through which the sun is

viewed. 

Prominences and active

regions will return as they

always have before.  

Sunspot

Sunspot

Maximum

Maximum

Sunspot

Sunspot

Minimum

Minimum

Summary of Contents for SolaREDi

Page 1: ...are rear mounted DayStar filter optics are designed to tilt for tuning DayStar filter optics have operative temperature ranges DayStar SolaREDi telescopes have LONG focal ratios Fast eyepeices such a...

Page 2: ...or remote operation international power supply and 6 foot extension cord Energy Rejection Filter Mounted on the front of the telescope before the objective a red or yellow colored glass Energy Rejecti...

Page 3: ...rface Stroke from the center of the aperture outward only After each cleaning stroke use a fresh applicator The fewer strokes the better The tube and other parts are powder coated for durability and c...

Page 4: ...cal surfaces Do not disturb your optical stack If a small amount of couplant is smudged onto your outer surfaces it is best not to disturb it It will not affect performance like a large mirror Larger...

Page 5: ...lly occur The DSLR imager must be aware that most camera manufacturers Canon and Nikon use an IR blocking filter which greatly reduces the transmission of Hydrogen Alpha light DSLR cameras without thi...

Page 6: ...igured TeleVue 4X Televue Powermate barlow lens a DayStar Filters sub angstrom bandpass Hydrogen Alpha filter assembly and TeleVue Sol Searcher solar finder Mounting The SolaREDi combination mounting...

Page 7: ...marked by pores or small developing sunspots Surges or even small solar flares can sometimes occur in EFRs An EFR emerges with small bright H region with little surges then weak arch filaments AFS ove...

Page 8: ...chromosphere surrounding the surface Using eyepieces higher than 12mm in power it is challenging to achieve focus on the limb For users who are interested in higher magnification we suggest one of our...

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