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\title{Multiwavelength modeling of the Vela pulsar pulses - from Optical light to VHE gamma-rays
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\author{\speaker{Bronislaw Rudak}\\
        Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences
 \\
        E-mail: \email{bronek@ncac.torun.pl
}}

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\abstract{
  The pulsed radiation from PSR B0833-45 (Vela) has a phased-averaged spectral 
energy distribution of an apparently simple structure across a wide energy range. 
However, in narrow energy bands the pulses reveal astonishing complexity of
the directional pattern of the radiation. We present the results of a 3D modeling 
of the Vela radiation properties in the outer-gap scenario. 
We show how the synchrotron emission as well as the inverse Compton scattering (ICS) 
of soft photons by secondary e$^\pm$-pairs in its magnetic and non-magnetic 
regimes reproduces qualitatively, and in some cases quantitatively, the observed 
energy-dependent pulses of Vela.
Moreover, we present how ICS of soft synchrotron photons by primary particles can 
form a pulsed spectral component in the VHE domain. The flux of this component
should be of interest to the Cherenkov Telescope Array.
}

\FullConference{7th Fermi Symposium 2017\\
		15-20 October 2017\\
		Garmisch-Partenkirchen, Germany}


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