DayStar Filters QUARK Quick Start Manual Download Page 2

Cautions & Warnings:  

 

There are n o use r se rviceable pa rts inside the  Quark.  Do not 

diassemble t he unit.  Certain 

components are  under p ressure a nd 

disassembly can ca use permanent  damage.  All el ements are required  

for proper operation and removal of any internal component will cause a 

malfunction that could result in unfiltered light which can cause blindness 

or damage to equipment. 

Solar Observing with a telescope is sensitive to certain risks.   

  Caution and  care of the telescop

e and filter is advised in

 

assembly, use and dismantling at all times.   

  Telescope owners must use caution when affixing the filter to the 

telescope ne ver to poi nt any telesco pe at the  sun without th e 

solar filter safely installed first.   

  While ob serving,  owners must  take care and ca ution  that  all 

parts of the filter and telescope a ssembly are pro perly affixed 

and th at no  pie ces h ave be en  opened, tam pered  with  or 

removed.   

 

Owners must also use caution 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 guest or novice 

observers of the special nature of the telescope configuration so 

not to imply that telescopi c observing of the sun is  safe without 

proper filtration.  

 

A few very important points that owners and operators must 
understand: 

 

DayStar filters are rear-mounted and can be applied to a 
choice of telescopes

 if  applie d p roperly. If app lication i s 

incorrect, the filter will not perform as specified. 

  DayStar Filters a re interferen ce filters.  

If light reaches a 

DayStar Filter at an angle, it will cause wavelength 
wingshift.   

For our application on a  telescope, DayStar owners 

need F/1 5 to  F/30 light, so we  need to alter you r  telescope’s 

F/ratio in order to reach  F/15 to  F/30 where your  DayStar  will 

operate correctly. Best performance is at F/27-F/32. 

 

DayStar filters are temperature sensitive.

  Changi ng the  

temperature will change the wavelength (CWL) that the filter will  

transmit.   Users need to be aware of temperature tuning issues. 

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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