Proceedings of Topical Meeting on Optoinformatics (pdf-format, 1.21 ...
Proceedings of Topical Meeting on Optoinformatics (pdf-format, 1.21 ... Proceedings of Topical Meeting on Optoinformatics (pdf-format, 1.21 ...
26 OPTOINFORMATICS’05 (b) Photoacoustic and photothermal measurements under annealing
SAINT-PETERSBURG, October 17 – 20, 2005 27 ESTIMATION OF INFLUENCE OF STATISTICAL ERRORS ON AN ACURACY OF CALIBRATION OF THE SPACE SOLAR PATROL INSTRUMENTATION AT A SYNCHROTRON RADIATION SOURCE Afanas’ev I.M., S.I. Vavilov State Optical Institute, Tuchkov lane, 1; St. Petersburg, 199034, Russia; e-mail: afanasy@rambler.ru In the article the values
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SAINT-PETERSBURG, October 17 – 20, 2005 27<br />
ESTIMATION OF INFLUENCE OF STATISTICAL ERRORS ON AN<br />
ACURACY OF CALIBRATION OF THE SPACE SOLAR PATROL<br />
INSTRUMENTATION AT A SYNCHROTRON RADIATION SOURCE<br />
Afanas’ev I.M., S.I. Vavilov State Optical Institute, Tuchkov lane, 1; St. Petersburg,<br />
199034, Russia; e-mail: afanasy@rambler.ru<br />
In the article the values <str<strong>on</strong>g>of</str<strong>on</strong>g> statistical errors, dealt with random character both<br />
emitting <str<strong>on</strong>g>of</str<strong>on</strong>g> synchrotr<strong>on</strong> radiati<strong>on</strong> (SR) in a storage ring, and registrati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> a<br />
SR by a receiving tract <str<strong>on</strong>g>of</str<strong>on</strong>g> the Space Solar patrol (SSP) instrumentati<strong>on</strong>, are<br />
evaluated.<br />
The SSP instrumentati<strong>on</strong> has been created to m<strong>on</strong>itor the i<strong>on</strong>izing radiati<strong>on</strong> from the<br />
Sun in the spectral range 0,14 – 198 nm from space apparatus. It c<strong>on</strong>sists <str<strong>on</strong>g>of</str<strong>on</strong>g> a Radiometer<br />
with 20 filters and two grating spectrometers [1] . The absolute spectral calibrati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> the<br />
SSP instrumentati<strong>on</strong> in the spectral range from 0,25 up to 122 nm (5000 - 10 eV) has been<br />
preparing by the special metrological stati<strong>on</strong>s at the SR sources <str<strong>on</strong>g>of</str<strong>on</strong>g> the storage rings<br />
VEPP-3 and VEPP-4 (at the G.I. Budker Institute <str<strong>on</strong>g>of</str<strong>on</strong>g> Nuclear Physics, Novosibirsk,<br />
Russia) [2] . All SSP measuring channels have "solar-blind" detectors – open sec<strong>on</strong>daryelectr<strong>on</strong><br />
multipliers (SEM), which have high sensitivity to radiati<strong>on</strong> below 160 nm [1] . The<br />
registrati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> radiati<strong>on</strong> by the SSP instrumentati<strong>on</strong> is realized with SEM in pulse mode.<br />
The aleatory variable <str<strong>on</strong>g>of</str<strong>on</strong>g> fluctuati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> counting rate f (which is the SSP output<br />
signal [3] ) is taken into account by the apparatus error σ app , which is distributed accordingly<br />
normal law. It is stipulated by random character both SR beam intensity I, and losses in the<br />
SSP registering channel η. [3] In the given calculati<strong>on</strong>, the losses are admitted to the<br />
c<strong>on</strong>stant value η=τ⋅γ=10 -4 electr<strong>on</strong>/phot<strong>on</strong> (thus, not taking into account their spectral<br />
character), where τ - effective transmissi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> the SSP channel (mainly, filters for the<br />
Radiometer and a polychromator for spectrometers; for both cases τ is about 10 -2 ) [4] , and γ<br />
- quantum efficiency <str<strong>on</strong>g>of</str<strong>on</strong>g> the SEM photocathode (average value is about 10 -2 ) [4] . Thus, the<br />
signal <str<strong>on</strong>g>of</str<strong>on</strong>g> counting rate will amount to f=I⋅η=10 4 pulses/sec, at the SR beam intensity I=10 8<br />
phot<strong>on</strong>/sec (see, table). The root-mean-square deviati<strong>on</strong> f from the expected aleatory<br />
variable f is "noise" <str<strong>on</strong>g>of</str<strong>on</strong>g> the SSP output signal, which hinders the measured signal the more,<br />
the lower value <str<strong>on</strong>g>of</str<strong>on</strong>g> a counting rate (i.e. the lower level a loading <str<strong>on</strong>g>of</str<strong>on</strong>g> a SSP registering<br />
channel).<br />
For unambiguous explanati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> calibrati<strong>on</strong> results it must be used the <strong>on</strong>e-electr<strong>on</strong><br />
mode at measurements. The two-electr<strong>on</strong> event is c<strong>on</strong>sidered as a certain hindering factor -<br />
"noise". It should be noticed, that the multi-electr<strong>on</strong> events at the given estimati<strong>on</strong> are not<br />
c<strong>on</strong>sidered. As a matter <str<strong>on</strong>g>of</str<strong>on</strong>g> fact, the ratio <str<strong>on</strong>g>of</str<strong>on</strong>g> probabilities <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>on</strong>e and two-electr<strong>on</strong> events<br />
P(1)/P(2) is the "signal-to-noise merit", inverse value <str<strong>on</strong>g>of</str<strong>on</strong>g> which is the statistical error σ stat .<br />
It is supposed, that probability distributi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> aleatory variable <str<strong>on</strong>g>of</str<strong>on</strong>g> appearing <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>on</strong>e,<br />
m −λ<br />
two, etc. photoelectr<strong>on</strong> events at experiment is described by the Poiss<strong>on</strong> law: λ ⋅e<br />
P(<br />
m)<br />
= ;<br />
m!<br />
where λ - expectati<strong>on</strong>, which is the multiplicati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> the SR beam intensity I<br />
(including its modulati<strong>on</strong> with frequency <str<strong>on</strong>g>of</str<strong>on</strong>g> circulati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> electr<strong>on</strong> beam f VEPP-4 at the<br />
VEPP-4 storage ring about 1 MHz) [3] by attenuati<strong>on</strong> losses at the registering tract η;<br />
m – value <str<strong>on</strong>g>of</str<strong>on</strong>g> acts <str<strong>on</strong>g>of</str<strong>on</strong>g> photoelectr<strong>on</strong> emissi<strong>on</strong> from the SEM photocathode (i.e.<br />
appearance <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>on</strong>e-electr<strong>on</strong> event (OEE) if m=1, two-electr<strong>on</strong> event (TEE) if m=2, etc).