CN108387317A - A kind of prism-type space heterodyne spectrograph - Google Patents
A kind of prism-type space heterodyne spectrograph Download PDFInfo
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- CN108387317A CN108387317A CN201810184071.XA CN201810184071A CN108387317A CN 108387317 A CN108387317 A CN 108387317A CN 201810184071 A CN201810184071 A CN 201810184071A CN 108387317 A CN108387317 A CN 108387317A
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- prism
- total reflection
- reflection mirror
- beam splitter
- dispersing
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- 238000003384 imaging method Methods 0.000 claims abstract description 15
- 230000003287 optical effect Effects 0.000 claims description 18
- 239000000463 material Substances 0.000 claims description 6
- 238000001514 detection method Methods 0.000 claims description 2
- 230000007423 decrease Effects 0.000 abstract description 4
- 239000006185 dispersion Substances 0.000 description 5
- 238000001228 spectrum Methods 0.000 description 5
- 238000004611 spectroscopical analysis Methods 0.000 description 4
- 230000001427 coherent effect Effects 0.000 description 2
- 238000010586 diagram Methods 0.000 description 2
- 238000005516 engineering process Methods 0.000 description 2
- 230000002452 interceptive effect Effects 0.000 description 2
- 230000007812 deficiency Effects 0.000 description 1
- 239000007789 gas Substances 0.000 description 1
- 238000000034 method Methods 0.000 description 1
- 230000000149 penetrating effect Effects 0.000 description 1
- 238000011084 recovery Methods 0.000 description 1
- 238000010183 spectrum analysis Methods 0.000 description 1
- 230000009466 transformation Effects 0.000 description 1
Classifications
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- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRARED, VISIBLE OR ULTRAVIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colours
- G01J3/28—Investigating the spectrum
- G01J3/2823—Imaging spectrometer
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRARED, VISIBLE OR ULTRAVIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colours
- G01J3/02—Details
- G01J3/0205—Optical elements not provided otherwise, e.g. optical manifolds, diffusers, windows
- G01J3/0208—Optical elements not provided otherwise, e.g. optical manifolds, diffusers, windows using focussing or collimating elements, e.g. lenses or mirrors; performing aberration correction
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRARED, VISIBLE OR ULTRAVIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colours
- G01J3/12—Generating the spectrum; Monochromators
- G01J3/14—Generating the spectrum; Monochromators using refracting elements, e.g. prisms
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRARED, VISIBLE OR ULTRAVIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colours
- G01J3/28—Investigating the spectrum
- G01J3/45—Interferometric spectrometry
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRARED, VISIBLE OR ULTRAVIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colours
- G01J3/12—Generating the spectrum; Monochromators
- G01J2003/1208—Prism and grating
Abstract
The invention discloses a kind of prism-type space heterodyne spectrographs, including incident diaphragm, collimation lens, beam splitter, the first dispersing prism, the second dispersing prism, the first total reflection mirror, the second total reflection mirror, imaging unit and detector, it is characterized in that, collimation lens and beam splitter are followed successively by rear side of the incidence diaphragm, the upside of the beam splitter is equipped with downside of the rear side of the first dispersing prism, the first total reflection mirror, beam splitter successively equipped with the second dispersing prism and the second total reflection mirror, beam splitter and is equipped with imaging unit and detector successively successively.This spectrometer has the advantages that super spectrally resolved, high-throughput, movement-less part, while being also avoided that in grating type space heterodyne spectrograph the problem of energy loss caused by grating multiorder diffractive, interference degree decline.
Description
Technical field
The present invention relates to optical remote sensing field of detecting, specifically a kind of prism-type space heterodyne spectrograph.
Background technology
Spatial heterodyne spectroscopy is to propose concept the 1970s, quick because of the progress of technical conditions to the nineties
A kind of spectral analysis technique of the novel achievable super-resolution to grow up, the technology have super spectrally resolved, high-throughput, nothing
The advantages that moving component.Spatial heterodyne spectroscopy can obtain high spectrally resolved in the wave-length coverage of a certain determination
Rate.The performance of spatial heterodyne spectroscopy brilliance makes it have distinctive feature in the super spectrographic detection of small-signal target, and answers
For the remote sensings of Atmospheric Trace Gases, the astronomical observation etc. of interstellar matter.
Traditional space heterodyne spectrograph carries out interference modulations by the way of grating beam splitting, however there are multistages to spread out for grating
It penetrates, generally use first-order diffraction light is then ignored as interfering beam, the diffraction light of other levels.Grating multiorder diffractive can cause
Problems with：On the one hand, the multiorder diffractive of grating can reduce the energy of interfering beam, be unfavorable for the spy of atomic dim light spectrum signal
It surveys；On the other hand, the diffraction light of other levels forms interferometer system internal stray light, largely reduces outside space
The interference degree of difference spectra instrument interference fringe, directly affects the precision of Fourier trasform spectroscopy.
Invention content
The purpose of the present invention is in view of the deficiencies of the prior art, and provide a kind of prism-type space heterodyne spectrograph.It is this
Spectrometer has the advantages that super spectrally resolved, high-throughput, movement-less part, while being also avoided that grating type space heterodyne spectrograph
In the energy loss caused by grating multiorder diffractive, interference degree decline the problem of.
Realizing the technical solution of the object of the invention is：
A kind of prism-type space heterodyne spectrograph, including incident diaphragm, collimation lens, beam splitter, the first dispersing prism, the second color
Dissipate prism, the first total reflection mirror, the second total reflection mirror, imaging unit and detector, unlike the prior art, the incidence
It is followed successively by collimation lens and beam splitter on rear side of diaphragm, the upside of the beam splitter is all-trans equipped with the first dispersing prism and first successively
Penetrate mirror, the rear side of beam splitter is equipped with the second dispersing prism successively and the downside of the second total reflection mirror, beam splitter is equipped with imaging successively
Unit and detector.
The beam splitter is semi-transparent semi-reflecting beam splitting element.
The material and appearance and size all same of first dispersing prism and the second dispersing prism, two dispersing prisms
Apex angle is identical angle.
The material and appearance and size all same of first total reflection mirror and the second total reflection mirror.
On the upside of the beam splitter and the first dispersing prism, the first total reflection mirror and the second dispersing prism of rear side two-arm and the
Two total reflection mirror positions are fixed, and the first total reflection mirror of two-arm and the second total reflection mirror face orthogonal with the optical axis are at identical
Overturning angle is placed, and the first dispersing prism of two-arm and the plane of incidence of the second dispersing prism are vertical with optical axis.
The distance at center to the beam splitter center of first dispersing prism and the second dispersing prism is equal.
The distance at center to the beam splitter center of first total reflection mirror and the second total reflection mirror is equal.
The detector is on the focal plane of imaging unit.
The detector is linear array or planar array detector.
Tested light beam penetrates diaphragm, and forms plane wave after collimated lens, is incident on beam splitter, is divided into intensity phase
Deng two beam coherent lights, respectively by being all-trans after the first dispersing prism of beam splitter two-arm and the light splitting of the second dispersing prism and through first
It penetrates mirror and the reflection of the second total reflection mirror returns to beam splitter, two outgoing beam corrugateds form the interference fringe of spatial modulation at angle,
It is imaged on detector eventually by imaging unit.
The fundamental frequency of the spectrometer can pass through the angle of dispersing prism and total reflection mirror and optical axis, the apex angle of dispersing prism
Carry out calculating acquisition.
Corrugated of the two-beam of the spectrometer fundamental frequency wavelength after dispersing prism and total reflection mirror return is vertical with optical axis,
With position phase, position difference is zero, does not generate interference fringe on two corrugateds；The light of non-fundamental frequency wave number is returned through dispersing prism and total reflection mirror
Afterwards, two outgoing wave faces face orthogonal with the optical axis forms angle, forms the space interference striped with fundamental frequency difference frequency；A certain monochrome
Two corrugateds of non-fundamental frequency wavelength will have an angle, and the optical path difference at center is zero, and the optical path difference at both ends is maximum；Interference fringe is imaged
Cell imaging is on detector.
The interference fringe that the spectrometer is recorded can restore the curve of spectrum of tested light after being fourier transformed.
The space heterodyne spectrograph of this structure uses two dispersing prism generations of the first dispersing prism and the second dispersing prism
Corrugated modulation is carried out for two diffraction grating in Traditional Space heterodyne spectrometer, prism-type space heterodyne spectrograph is by two dispersions
Light beam forms interference fringe, and the spatial frequency of interference fringe depends on the difference on the frequency between incident light and the specific fundamental frequency of system, is formed
Frequency difference interference, interference fringe are fourier transformed recovery spectrum.
The advantages of the technical program, is：
（1）Prism-type space heterodyne spectrograph inherits the key property of traditional raster type space heterodyne spectrograph, has ultraphotic
Compose resolution, high throughput, movement-less part etc..
（2）Prism-type space heterodyne spectrograph effectively prevents in grating type space heterodyne spectrograph since grating multistage is spread out
The problem of energy loss caused by penetrating and interference degree decline.
（3）Prism-type space heterodyne spectrograph carries out light splitting modulation using dispersing prism, compared with traditional raster type space heterodyne
Spectrometer design is simpler, cost is lower.
This spectrometer has the advantages that super spectrally resolved, high-throughput, movement-less part, while being also avoided that grating type sky
Between the problem of energy loss caused by grating multiorder diffractive, interference degree decline in heterodyne spectrometer.
Description of the drawings
Fig. 1 is the structural schematic diagram of the optical system of embodiment；
Fig. 2 is the interference fringe modulation principle schematic diagram in embodiment.
In figure, 1. diaphragm, 2. colimated light system, 301. first dispersing prism, 302. second dispersing prism 401. first is all-trans
Penetrate 6. imaging unit of mirror 402. second total reflection mirror, 5. beam splitter, 7. detector.
Specific implementation mode
The content of present invention is further elaborated with reference to the accompanying drawings and examples, but is not limitation of the invention,
Embodiment：
Referring to Fig.1, a kind of prism-type space heterodyne spectrograph, including incident diaphragm 1, collimation lens 2, beam splitter 5, the first dispersion
Prism 301, the second dispersing prism 302, the first total reflection mirror 401, the second total reflection mirror 402, imaging unit 6 and detector 7, with
Unlike the prior art, 1 rear side of incidence diaphragm is followed successively by collimation lens 2 and beam splitter 5, the upside of the beam splitter 5
The rear side for being equipped with the first dispersing prism 301 and the first total reflection mirror 401, beam splitter successively is equipped with the second dispersing prism 302 successively
It is equipped with imaging unit 6 and detector 7 successively with the downside of the second total reflection mirror 402, beam splitter 5.
The beam splitter 5 is semi-transparent semi-reflecting beam splitting element.
The material and appearance and size all same of first dispersing prism, 301 and second dispersing prism 302, two dispersions
The apex angle of prism is identical angle.
The material and appearance and size all same of first total reflection mirror, 401 and second total reflection mirror 402.
The first dispersing prism 301, the first total reflection mirror 401 and the second dispersion of 5 upside of the beam splitter and rear side two-arm
Prism 302 and 402 position of the second total reflection mirror are fixed, the first total reflection mirror 401 of two-arm and the second total reflection mirror 402 with
Optical axis normal surface is placed at identical overturning angle, the plane of incidence of the first dispersing prism 301 and the second dispersing prism 302 of two-arm
It is vertical with optical axis.
The distance at center to 5 center of beam splitter of first dispersing prism, 301 and second dispersing prism 302 is equal.
The distance at center to 5 center of beam splitter of first total reflection mirror, 401 and second total reflection mirror 402 is equal.
The detector 7 is on the focal plane of imaging unit 6.
The detector 7 is linear array or planar array detector, and this example is planar array detector.
As shown in Fig. 2, tested light beam penetrates diaphragm 1, and plane wave is formed after collimated lens 2, is incident on beam splitter 5
On, it is divided into two equal beam coherent lights of intensity, respectively by the first dispersing prism 301 of 5 two-arm of beam splitter and the second dispersion rib
Beam splitter 5, two outgoing beam corrugateds are returned to after mirror 302 is divided and through the first total reflection mirror 401 and the reflection of the second total reflection mirror 402
At angle, the interference fringe of spatial modulation is formed, is imaged on detector 7 eventually by imaging unit 6.
The fundamental frequency of the spectrometer can pass through the angle of dispersing prism and total reflection mirror and optical axis, the apex angle of dispersing prism
And the refractive index n of dispersing prism carries out calculating acquisition, can be derived by general geometric optics.
Corrugated of the two-beam of the spectrometer fundamental frequency wavelength after dispersing prism and total reflection mirror return is vertical with optical axis,
With position phase, position difference is zero, does not generate interference fringe on two corrugateds；The light of non-fundamental frequency wave number is returned through dispersing prism and total reflection mirror
Afterwards, two outgoing wave faces face orthogonal with the optical axis forms angle, forms the space interference striped with fundamental frequency difference frequency；A certain monochrome
Two corrugateds of non-fundamental frequency wavelength will have an angle, and the optical path difference at center is zero, and the optical path difference at both ends is maximum；Interference fringe is imaged
Unit 6 images on detector 7.
Two-beam will interfere, and form equal thick interference fringe.The imaged object lens of interference fringe image in linear array detector 7
On, the interference fringe at different location is recorded, and the curve of spectrum to be measured can be calculated by Fourier transformation.
Claims (9)
1. a kind of prism-type space heterodyne spectrograph, including incident diaphragm, collimation lens, beam splitter, the first dispersing prism, second
Dispersing prism, the first total reflection mirror, the second total reflection mirror, imaging unit and detector, characterized in that on rear side of the incidence diaphragm
It is followed successively by collimation lens and beam splitter, the upside of the beam splitter is equipped with the first dispersing prism, the first total reflection mirror, beam splitting successively
The rear side of device is equipped with the second dispersing prism successively and the downside of the second total reflection mirror, beam splitter is equipped with imaging unit and detection successively
Device.
2. prism-type space heterodyne spectrograph according to claim 1, characterized in that the beam splitter is semi-transparent semi-reflecting
Beam splitting element.
3. prism-type space heterodyne spectrograph according to claim 1, characterized in that first dispersing prism and
The material of two dispersing prisms and the apex angle of appearance and size all same, two dispersing prisms are identical angle.
4. prism-type space heterodyne spectrograph according to claim 1, characterized in that first total reflection mirror and second
The material and appearance and size all same of total reflection mirror.
5. prism-type space heterodyne spectrograph according to claim 1, characterized in that the beam splitter upside and rear side two
The first dispersing prism, the first total reflection mirror and the second dispersing prism of arm and the second total reflection mirror position are fixed, two-arm
First total reflection mirror and the second total reflection mirror face orthogonal with the optical axis are placed at identical overturning angle, the first dispersing prism of two-arm
It is vertical with optical axis with the plane of incidence of the second dispersing prism.
6. prism-type space heterodyne spectrograph according to claim 1, characterized in that first dispersing prism and second
The distance at the center of dispersing prism to beam splitter center is equal.
7. prism-type space heterodyne spectrograph according to claim 1, characterized in that first total reflection mirror and second
The distance at the center of total reflection mirror to beam splitter center is equal.
8. prism-type space heterodyne spectrograph according to claim 1, characterized in that the detector is in imaging unit
On focal plane.
9. prism-type space heterodyne spectrograph according to claim 1, characterized in that the detector is linear array or face battle array
Detector.
Priority Applications (1)
| Application Number | Priority Date | Filing Date | Title |
|---|---|---|---|
| CN201810184071.XA CN108387317A (en) | 2018-03-06 | 2018-03-06 | A kind of prism-type space heterodyne spectrograph |
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| Application Number | Priority Date | Filing Date | Title |
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| CN201810184071.XA CN108387317A (en) | 2018-03-06 | 2018-03-06 | A kind of prism-type space heterodyne spectrograph |
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Cited By (3)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| CN109764963A (en) * | 2019-01-23 | 2019-05-17 | 桂林电子科技大学 | A kind of setting of prism-type space heterodyne spectrograph reference wavelength and adjustment method |
| CN112067598A (en) * | 2020-09-15 | 2020-12-11 | 江苏师范大学 | Low-noise spatial heterodyne spectrometer for short-wave ultraviolet Raman spectrum detection |
| CN112504457A (en) * | 2020-11-27 | 2021-03-16 | 武汉船舶通信研究所（中国船舶重工集团公司第七二二研究所） | Spatial heterodyne spectrometer applied to DWDM system |
Citations (4)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| US7330267B1 (en) * | 1999-04-09 | 2008-02-12 | Campus Technologies Ag | Device and method for optical spectroscopy |
| US20090231592A1 (en) * | 2008-03-17 | 2009-09-17 | Harlander John M | Refractive spatial heterodyne spectrometer |
| CN102052968A (en) * | 2010-11-29 | 2011-05-11 | 中国科学院西安光学精密机械研究所 | Wide-spectrum spatial heterodyne spectrometer |
| CN207976221U (en) * | 2018-03-06 | 2018-10-16 | 桂林电子科技大学 | A kind of prism-type space heterodyne spectrograph |
-
2018
- 2018-03-06 CN CN201810184071.XA patent/CN108387317A/en active Pending
Patent Citations (4)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| US7330267B1 (en) * | 1999-04-09 | 2008-02-12 | Campus Technologies Ag | Device and method for optical spectroscopy |
| US20090231592A1 (en) * | 2008-03-17 | 2009-09-17 | Harlander John M | Refractive spatial heterodyne spectrometer |
| CN102052968A (en) * | 2010-11-29 | 2011-05-11 | 中国科学院西安光学精密机械研究所 | Wide-spectrum spatial heterodyne spectrometer |
| CN207976221U (en) * | 2018-03-06 | 2018-10-16 | 桂林电子科技大学 | A kind of prism-type space heterodyne spectrograph |
Cited By (5)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| CN109764963A (en) * | 2019-01-23 | 2019-05-17 | 桂林电子科技大学 | A kind of setting of prism-type space heterodyne spectrograph reference wavelength and adjustment method |
| CN109764963B (en) * | 2019-01-23 | 2020-12-04 | 桂林电子科技大学 | Reference wavelength setting and debugging method for prism type spatial heterodyne spectrometer |
| CN112067598A (en) * | 2020-09-15 | 2020-12-11 | 江苏师范大学 | Low-noise spatial heterodyne spectrometer for short-wave ultraviolet Raman spectrum detection |
| CN112504457A (en) * | 2020-11-27 | 2021-03-16 | 武汉船舶通信研究所（中国船舶重工集团公司第七二二研究所） | Spatial heterodyne spectrometer applied to DWDM system |
| CN112504457B (en) * | 2020-11-27 | 2023-02-24 | 武汉船舶通信研究所（中国船舶重工集团公司第七二二研究所） | Spatial heterodyne spectrometer applied to DWDM system |
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