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26 . System Description
For operation in the ultraviolet (UV) range, mirror M1 is raised to permit radiation from the
deuterium lamp to strike source mirror M2. Source change is automatic during
monochromator slewing.
Radiation from the respective source lamp is reflected from mirror M2 via mirror M3 through
an optical filter on the filter wheel assembly (FW) to mirror M4.
The filter wheel is driven by a stepping motor to be in synchronization with the
monochromators. Depending on the wavelength being produced, the appropriate optical
filter is located in the beam path to prefilter the radiation before it enters the
monochromator. Filter change is automatic during monochromator slewing.
From mirror M4 the radiation is reflected through the entrance slit of Monochromator I. All
slits are located on the slit assembly (SA). The radiation is collimated at mirror M5 and
reflected to the grating table G1. Depending on the current wavelength range, the collimated
radiation beam strikes either the UV/Vis grating or the NIR grating (NIR version only).
The radiation is dispersed at the grating to produce a spectrum. The rotational position of
the grating effectively selects a segment of the spectrum, reflecting this segment to mirror
M5 and then through the exit slit. The exit slit restricts the spectrum segment to a near-
monochromatic radiation beam. Grating change is automatic during monochromator slewing.
The exit slit of Monochromator I serves as the entrance slit of Monochromator II. The
radiation is reflected via mirror M6 to the appropriate grating on grating table G2 and then
back via mirror M6 through the exit slit to Mirror M7. The rotational position of grating table
G2 is synchronized to that of G1. The radiation emerging from the exit slit exhibits high
spectral purity with an extremely low stray radiation content.
In the UV/Vis and NIR range a choice is provided between a fixed slit width, a servo slit, and
a slit program. When the servo slit is selected, the slit widths change automatically during
scanning to maintain constant energy at the detector.
From mirror M7 the radiation beam is reflected via toroid mirror M8 to the chopper assembly
(C). As the chopper rotates, a mirror segment, a window segment and two dark segments
are brought alternately into the radiation beam.
When a window segment enters the beam, radiation passes through to mirror M9 and is then
reflected via mirror M10 to create the reference beam (R).
When a mirror segment enters the beam the radiation is reflected via mirror M10
΄
to form
the sample beam (S).
When a dark segment is in the beam path, no radiation reaches the detector, permitting the
detector to create the dark signal.
The radiation passing alternately through the sample and reference beams is reflected by
mirrors M11, M12, M13, and M11
΄
, M12
΄
, M13
΄
, respectively of the optics in the detector
assembly onto the appropriate detector. Mirror M14 is rotated to select the required detector.
A photomultiplier (PM) is used in the UV/Vis range while a lead sulfide (PbS) detector is used
in the NIR range. Detector change is automatic during monochromator slewing.
At the cell plane, each radiation beam is approximately 12 mm high. The width of the
radiation beams is dependent on the slit width. At a slit width of 5 nm each radiation beam is
approximately 4.5 mm wide.
Содержание Lambda 650
Страница 1: ...LAMBDA 650 850 950 Hardware Guide UV VIS SPECTROSCOPY ...
Страница 5: ...Introduction ...
Страница 10: ...10 Introduction ...
Страница 11: ...Safety Practices ...
Страница 23: ...System Description ...
Страница 32: ...32 System Description ...
Страница 33: ...Lambda 650 Installation ...
Страница 44: ...44 Lambda 650 Installation ...
Страница 45: ...Using the Instrument ...
Страница 54: ...54 Using the Instrument ...
Страница 55: ...Maintenance ...
Страница 72: ...72 Maintenance ...