DayStar Filters QUARK Quick Start Manual Download Page 5

 

How it works: 

 

Light fro m t he tele scope enters th e blo cking filter  (at left),  where 

wavelengths  near H alph a are  tran smitted whil e the  re st are reflected  

back out.  Red H  alpha light then p asses through the tele centric barlow 

lens elements to  achieve a slower focal ratio, m ore parallel light beam.  

The Etalon p asses a very narrow rang e of light wavelength s, but it is 

sensitive to t emperature  and lig ht an gle.  In the   Quark, the  Etalon is 

heated to a pproximately  100-150°F to  co ntrol the  wavelength  passed, 

and the telecentric barlow controls the angle of light entering the Etalon. 

 

Care and cleaning:

 

 

 

While not in use, we re commend that users store the Quark with its end 

caps on, in  a climate controlled e

nvironment. The optical filter life

 

expectancy is extended up to 2-3 times by climate controlled storage. 

 

Do not touch the internal,  optical elements of the  filter a ssembly. While 

the exterio r glass  surface  coatings a re d urable, they are ea

sily 

scratched. A  few specks of dust will have no effect  on the quality of th e 

image, and may be g ently blown off with a sque eze bulb.  Do NOT use 

compressed  air can s to  blow  dust off any optical  surfa ces. S mall 

amounts of residual 'film' will not affect visual performance. Fingerprints, 

smudges and smears must be cleaned off. Preferred cleaning met hod is 

to return the  Quark to the DayStar  Filters la boratory for prope r factory 

cleaning. 

 

Do not unscrew, open or separate your Quark filter assembly. The optical 

elements are held under pressure by design and will become damaged if 

opened. Opening the opti cal filter asse mbly will void  your wa rranty. The 

safest cleaning method is to moisten  a very soft, lint-free tissue, cloth or  

"Qtip" with a  pure  acetone, methan ol, or Iso propyl Alcohol  (reagent 

grade) and gently whisk away the stain. Do not apply solutions directly to 

the glass surface. Stroke from the  center of the ape rture outward only. 

After each cleaning stroke, use a fresh applicator. The fewer strokes, the 

better! The  metal hou sing and othe r non optical  parts are a nodized 

surfaces and can be cleaned with Windex. 

Summary of Contents for QUARK

Page 1: ...t damage we recommend using an Energy Rejection Filter on telescopes of 80mm aperture or more or when tra cking the Sun for long periods This can be a UV IR cut filter mounted before the diagonal or a...

Page 2: ...n when the telescope is being assembled and dismantled to assure the telescope is never pointing at the sun without the solar filter properly installed Responsible owners will be prud ent to inform gu...

Page 3: ...la cks contrast you may nee d t o adj ust th e ce nter wavelength of the filter A knob is provided to adjust the center wavelength of the filter Turn th e knob counter clockwise to lower the waveleng...

Page 4: ...h oil spaced o bjective tele scopes or any telescope with an integrated rear field flattener or Petzval lens The UV IR cut filter must be the first optical element to receive concentrated light For b...

Page 5: ...rable they are ea sily scratched A few specks of dust will have no effect on the quality of th e image and may be g ently blown off with a sque eze bulb Do NOT use compressed air can s to blow dust of...

Page 6: ...t m ost even view and wid est exit pupil In Solar Observing contrast is achieved by co ntrol of scattering Tele Vue Plossl s stand out in superior design Furthermore the adjustable eye cup offers addi...

Page 7: ...eing conditions even on a clear day DayStar Filters are high power viewing platforms and this high resolution can b e su sceptible to seei ng issu es Solar Ob servers usi ng high powered hig h resolut...

Page 8: ...y 1 in 4 pi xels detect red light The other 3 sensors only detect blue and green b ecause the p ixels are a ctually permanently covered with a colored dye for each corresponding color So a co lor CCD...

Page 9: ...ange from bright solar flares to faint eruptive or floating prominences quite a distance from the solar limb In order to capture all these features we recommend the use of 12 bit or 16 bit cameras Nor...

Page 10: ...ast of space To observe the details of chromosphere on the face of the sun we ne ed a narrower fil ter to elimin ate more off band li ght of the photosphere and continuum We need a filter l ess tha n...

Page 11: ...several ty pes of features co ntained in a close area Field Transition Arches FTA s connect P and F spots ele ments of opposite polarity Inside a n active region w here sunspots a re originally linked...

Page 12: ...re sses in line s of force b uild up slowly a nd a re released in flares They occur mo st freque ntly at n eutral li nes where a fila ment is supported by hori zontal sheared field lines Thi s e vent...

Page 13: ...g Try moving to a different location or else observe on a day when weather conditions are improved Yellow LED indication Your filter i s adjusting to t he wavelen gth ch osen by the kn ob Wait approxi...

Page 14: ...and 2 0 combo male snouts with safety indent Focal point 1 25 snout requires approx 8mm in focus 2 requires approx 10mm out focus Eyepiece side 1 25 female drawtube Brass compression ring to protect...

Page 15: ...e ceiver C nt from that to w experienced radio This Product al Electronic Eq the Eu ropean separate collectio shown o n the pr o ot be disposed w e To preve nt pos ncontrolled waste stes and recy cle...

Page 16: ...ranty at any time while this warranty is in effect warrantor will repair the defect and return it to you without charge for parts service or any cost incurred by the warrantor in connection with the p...

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