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A N A L I S I E M N U M E R I C A D I P U P I L L E T O R A L D O
P. B O L L I ( I N A F - O A A )
Super resolving systems: Toraldo Pupils (PUTO Project)
Villa Galileo, Firenze, 12 Ottobre 2017
AGENDA
• Tools: Software (FEKO) and hardware
• Problems encountered to match the EM simulations to the TP analytical
description and definition of the EM model
• Simplified model for describing the super-resolution with respect to the
analytical model
• Simulations for comparison with the anechoic chamber measurements
• Collimator for the Medicina radio telescope
• Continuous TP
FEKO 1/2
FEKO (from Altair) is a comprehensive computational electromagnetics
code used widely in the telecommunications, automobile, space and
defense industries.
The MoM is a full wave solution of Maxwell's
integral equations in the frequency domain.
“Source method" only the structure in
question is discretized
No boundary conditions
Memory requirements (N2) scale proportional to
the size of the geometry in question (N) and the
required solution frequency.
FEKO 2/2
• Planar Green Functions for Multilayered Media: Planar Green’s Function to model the aperture
• Surface Equivalence Principle (SEP): The SEP introduces equivalent electric and magnetic currents
on the surface of a closed dielectric body
• Higher Order Basis Functions (HOBF): use higher order polynomial basis functions to model the
currents on any particular mesh element. Such HOBF allow the user to mesh geometry with larger
triangles, while obtaining the same solution accuracy.
• Multilevel fast multipole method (MLFMM): The MLFMM differs from the MoM in that it groups
basis functions and computes the interaction between groups of basis functions, rather than between
individual basis functions. Memory requirement: N2 N*log(N)
• Distributed/Shared Memory Hybridisation Optimized
• Lua Scripting and Automation
HARDWARE
• Deskotp
Windows 7 professional (64 bit)
XEON E3-1275v2 (3.5 GHz) – RAM=32 GB / Core=4 / Threads=8
Single-user
• Workstation
CentOS 7 (64 bit)
2 x XEON E5-2680v2 (2.8 GHz) – RAM=64 GB / Core=20 / Threads=40 (max 32 due to the FEKO
license)
Shared-user
Workstation vs desktop: 3-4 reduction factor in the computational time (if 32 GB RAM is enough)
One network license (3 keuro/year) with no simultaneous use
DISCRETE TP: ANALYTIC MODEL
DEFINIZIONE MODELLO EM
• Onda piana incidente soddisfa la condizione di fase, ma crea problemi di
diffrazione dal bordo esterno del disco metallico
• Si è quindi passati alla sorgente SWE (espansione onda sferica) gaussiana
(-14 dB @ 21.4 gradi). La sorgente deve essere posta lontana per avere
una quasi-onda piana nella PT, ma non troppo per non sovra-illuminare il
bordo
• Si è infine consolidata la soluzione del planar multi-layer
substrate con onda piana
ALTRI PARAMETRI EM • Frequenza 20 GHz miglior compromesso tra dimensioni fisiche contenute e
tempi di calcolo non eccessivi. Inoltre strumentazione RF presente in laboratorio
• Oggetti dielettrici (TP e lenti) di polietilene: costante dielettrica 2.278 e zero perdite ohmiche
• Inversione di fase (ritardo 180 gradi): spessore dielettrico circa l
• Conduttori elettrici perfetti
• Moarse mesh (λ/8)
• Onda piana polarizzata linearmente
• Laddove possibile utilizzati piani di simmetria elettrico e magnetico
• Pattern ottenuti in far-field o near-field (o matrice di scattering)
TP3
TP4
MODELLO SEMPLIFICATO TP3 • Principio sovrapposizione del campo irradiato da ciascun anello
• Approccio ha permesso di comparare simulazioni con modello teorico
• Inoltre considerare apodizzazione e tunare la fase della PT
R=1.5 cm
Fase = 0 deg
Amp = 1 V/m
Ri=3 cm; Re=4.5 cm
Fase = 0 deg
Amp = 1 V/m (0.23 V/m)
Ri=1.5 cm; Re=3 cm
Fase = 180 deg
Amp = 1 V/m (0.63 V/m)
RISULTATO TP3 - fase ideale
Rossa: teoria
Nera: FEKO
TP3 - fase con
dielettrico
Rossa: teoria
Nera: FEKO
1.7 cm
No apodizzazione Con apodizzazione
RISULTATO Ottimizzazione
spessore dielettrico
della corona 1 della
TP4
LABORATORY MEASUREMENT
EXP. ASTRONOMY RESULTS 1/2 Camera anecoica di Arcetri
Linear scanning in near-field
Matrice di scattering senza «probe compensation»
Misure
senza TP3
Misure con
TP3
FEKO
con TP3
Fig. 7, Exp Astron (2017) 43:285–309
EXP. ASTRONOMY RESULTS 2/2 Camera anecoica di IFAC
Plane-rectangular NF-FF transformation (UNISA)
Simulazioni FEKO in FF
Figs. 13 e 14, Exp Astron (2017) 43:285–309
NOT-NORMALIZED PATTERN & TP4 ISSUE TP4 invertita
(in accordo a teoria)
TP4 misurata in lab
COLLIMATORE PER MEDICINA
Aperture excitation (corresponding to the
Cassegrain focus): the focal plane field produced by
a plane wave reflected by the Medicina primary
mirror
First lens to convert the sphercial wave to a plane
wave
Aperure with Toraldo Pupil
Second lens to convert the plane wave to a
sphercial wave towards the new focus
New focal position
PIANO TP
52.5 42 21 8.75 52.5 42 21 8.75
PUPILLA CONTINUA
CONCLUSIONS
• Quite good knowledge of FEKO and specifically of this specific problem
• Nice tool for better understanding the physics behind the model and
predicting possible problems in the experimental set up (especially in view of
the installation at the Medicina RT)
• Simulation data have contributed in publishing the TP results
• Workstation very useful to run simulations in a reasonable time
• More systematic approach