scholarly journals Reduction of CCD observations made with a scanning Fabry–Perot interferometer. III. Wavelength scale refinement

2015 ◽  
Vol 70 (4) ◽  
pp. 494-500 ◽  
Author(s):  
A. V. Moiseev

A high-resolution photoelectric spectrometer employing a mechanically scanned Fabry - Perot interferometer is described. The spectrometer produces high-finesse spectral profiles continuously and rapidly at repetitive frequencies of up to 1000 c/s corresponding to a time resolving limit of 4 u s for a scan of 5 orders. The display is on an oscilloscope or a pen-recorder function-plotter. The instrument has been tested with the high-frequency discharge spectrum of mercury. Single intensity measurements are reproducible to better than 0.5%. The wavelength scale is linear to 0.5% over an order and can be corrected to four times this accuracy. Hyperfine structures agree well with recent determinations which use both pressure scanned and photographic Fabry-Perot systems. The mercury isotope abundances have been obtained from the spectral intensity measurements agreeing well with mass-spectrometer values. The r.m.s. deviation for a single determination is less than 0.5% of the percentage abundance. Possible applications to rapidly varying phenomena in gas discharges and shock waves, the determination of refractive indices and extension to the ultra-violet region for spectroscopy from an earth satellite are briefly considered.


Sensors ◽  
2020 ◽  
Vol 20 (21) ◽  
pp. 6304
Author(s):  
Aleksandr Markvart ◽  
Leonid Liokumovich ◽  
Iurii Medvedev ◽  
Nikolai Ushakov

Smartphone-based optical spectrometers allow the development of a new generation of portable and cost-effective optical sensing solutions that can be easily integrated into sensor networks. However, most commonly the spectral calibration relies on the external reference light sources which have known narrow spectral lines. Such calibration must be repeated each time the fiber and diffraction grating holders are removed from the smartphone and reattached. Moreover, the spectrometer wavelength scale can drift during the measurement because of the smartphone temperature fluctuations. The present work reports on a novel spectral self-calibration approach, based on the correspondence between the light wavelength and the hue features of the spectrum measured using a color RGB camera. These features are caused by the nonuniformity of camera RGB filters’ responses and their finite overlap, which is a typical situation for RGB cameras. Thus, the wavelength scale should be externally calibrated only once for each smartphone spectrometer and can further be continuously verified and corrected using the proposed self-calibration approach. An ability of the plug-and play operation and the temperature drift elimination of the smartphone spectrometer was experimentally demonstrated. Conducted experiments involved interrogation of optical fiber Fabry-Perot interferometric sensor and demonstrated a nanometer-level optical path difference resolution.


1982 ◽  
Vol 259 ◽  
pp. 900 ◽  
Author(s):  
F. L. Roesler ◽  
J. L. Lowrance ◽  
P. Zucchino ◽  
D. Long ◽  
R. J. Oliversen ◽  
...  

2014 ◽  
Vol 115 (10) ◽  
pp. 104504 ◽  
Author(s):  
Zhou Lin ◽  
Xiasheng Guo ◽  
Juan Tu ◽  
Jianchun Cheng ◽  
Junru Wu ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 593-596
Author(s):  
O. Bouchard ◽  
S. Koutchmy ◽  
L. November ◽  
J.-C. Vial ◽  
J. B. Zirker

AbstractWe present the results of the analysis of a movie taken over a small field of view in the intermediate corona at a spatial resolution of 0.5“, a temporal resolution of 1 s and a spectral passband of 7 nm. These CCD observations were made at the prime focus of the 3.6 m aperture CFHT telescope during the 1991 total solar eclipse.


1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


2000 ◽  
Vol 10 (PR8) ◽  
pp. Pr8-251
Author(s):  
L. Menez ◽  
I. Zaquine ◽  
A. Maruani ◽  
R. Frey
Keyword(s):  

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