L03_detectx

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    Detection of X-Rays

    Detector characteristics

    Proportional counters

    Microchannel plates

    Solid state detectors

    Microcalorimeters

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    Detector Characteristics

    Sensitivity

    Quantum efficiency Energy resolution

    Time resolution

    Position resolution

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    Sensitivity Fluctuations in background signal:

    B1is particle background

    is detector solid angle

    Ais detector effective area

    AB2is rate of X-ray background tis integration time

    Sis source flux (counts cm-2s-1)

    21 ABBtN

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    Sensitivity

    Signal to noise ratio of source detection

    Limiting sensitivity

    tABtB

    SAtn

    21

    AtBABS n

    21min

    /

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    Proportional Counter

    X-ray enters counter, interacts with gas emitting photoelectrons

    which drift toward anode

    E field near anode is high, electrons are accelerated and ionized

    additional atoms, original charge is multiplied

    Output is one electrical pulse per interacting X-ray

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    Energy ResolutionNumber of initial photoelectronsN=E/w, whereE= energy of X-

    ray, w= average ionization energy (26.2 eV for Ar, 21.5 eV for Xe)

    Creation of photoelectrons is a random process, number fluctuates

    Variance of N: N2=FN, whereFis the Fano factor, fluctuations

    are lower than expected from Poisson statistics (F

    = 0.17 for Ar, Xe)Energy resolution (FWHM) is

    E

    wF

    NE

    E N

    35.235.2

    Energy resolution is usually worse because of fluctuations

    in multiplication

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    Position Sensing

    Need to have drift E field which is parallel

    Readout anodes or cathodes are segmemted or crossed

    wires are used

    Resolution is limited by diffusion of electron cloud

    Time resolution is limited by drift time

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    SXRP Proportional Counter

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    Quantum Efficiency

    To be detected, X-ray must pass through window

    without being absorbed and then be absorbed in gas

    gw

    w dtTQ

    exp1exp

    Twis geometric open fraction of window, tis windowthickness, dis gas depth, s are absorption length for

    window/gas (energy dependent)

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    Efficiency versus Energy

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    Microchannel Plates

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    Microchannel Plates

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    Solid State X-ray Detectors

    X-ray interacts in material to produce photoelectrons

    which are collected by applying a drift field

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    Charge Coupled Devices

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    Charge Coupled Devices

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    1

    2

    3

    +5V

    0V

    -5V

    +5V

    0V

    -5V

    +5V

    0V

    -5V

    Time-slice shown in diagram

    1

    2

    3

    Charge Transfer in CCDs

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    Frame Store CCD

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    Pixelated Detectors

    CCDs have small pixel sizes,good energy resolution, and a

    single readout electronics

    channel, but are slow, thin (< 300

    microns), and only made in Si.Pixelated detectors have larger

    pixel sizes, require many

    electronics channels, but are fast

    and can be made thick and ofvarious materialstherefore can

    be efficient up to higher energies

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    Energy ResolutionEnergy resolution obeys same equation as for proportional counters,

    but average ionization energy is much smaller than for gases

    Material w (eV) Fano

    factor

    E@

    6 keV (eV)

    Ar 26.2 0.17 600-1200

    Xe 21.5 0.17 600-1200

    Si 3.62 0.115 120-250

    Ge 2.96 0.13 112

    CdTe 4.4 0.11 130-2000

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    Microcalorimeters

    E = 6 eV

    @ 6 keV

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    X-Ray Reflectivity

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    Grazing Incidence Optics

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    Scientific Gains from Imaging

    Increase S/N and thus sensitivity

    Reduce source area and thus the associated background

    Allow more accurate background estimation

    Take background events from the immediate vicinity of asource

    Enable the study of extended objects

    Structures of SNR, clusters of galaxies, galaxies, diffuseemission, jets,

    Minimize source confusion E.g., source distribution in galaxies

    Provide precise positions of sources

    Identify counterparts at other wavelengths

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    Gratings

    d

    m sinsin

    = incidence angle, = diffraction angle, = wavelength, m =

    diffraction order (1, 2, ), d= groove spacing

    For X-ray diffraction needd~ 0.11 m

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    Gratings

    http://space.mit.edu/CSR/hetgs_diagram.gif
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    Chandra

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    Reading

    Longair: 6.4, 6.5, 7.1, 7.3