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  <title>Prof.</title>
  <name first="Eduardo" middle="" last="Ros"></name>
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<title>Dissecting the Universe - Workshop on Results from High-Resolution VLBI</title>
<description>&lt;p&gt;&lt;img alt="" src="https://events.mpifr-bonn.mpg.de/indico/event/4/material/0/0.png" style="height:430px; width:720px" /&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Scientific rationale:&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;Recent developments have pushed the limits of resolution in astrophysics to new frontiers. Very-long-baseline interferometry (VLBI) at millimetre wavelengths or using antennas in space yields resolutions down to tens of microarcseconds (that is, fractions of nanoradians). These observations probe compact objects such as the innermost regions of active galactic nuclei. Space VLBI is living a new era at present with the results from the RadioAstron mission, enhancing radio interferometry in terms of resolution at least one order of magnitude with respect to ground-based VLBI. Millimetre VLBI also brings radio interferometry to a new range of resolution and with much enhanced sensitivity due to improvements in data bit rate. With more antennas capable of VLBI at 3-mm wavelength, and successful observations being carried out at 1-mm, a new window is open to universe at unprecedented resolution. This workshop will review recent results on high resolution radio astronomy, including opportunities provided by new antennas becoming available. It will also discuss on the applications of high-resolution imaging techniques and the synergies in the study of compact objects by space and mm-VLBI together.&amp;nbsp;&lt;/p&gt;

&lt;p&gt;Contributions to the workshop will be published online in this webpage; no regular proceedings are planned.&amp;nbsp; Abstracts will be sent to the Astrophysical Data System.&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Scientific Organising Committee:&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;E. Ros (MPIfR; Chair), M. Giroletti (IRA-INAF), T. Hovatta (Aalto Univ.), Y.Y. Kovalev (ASC Lebedev), A.P. Lobanov (MPIfR), J.A. Zensus (MPIfR)&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Local Organising Committee:&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;E. Ros (Chair), G. Bruni, B. Naunheim, J.A. Zensus&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Sponsors:&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;This meeting is sponsored by the MPI f&amp;uuml;r Radioastronomie and by &lt;a href="http://www.radionet-eu.org/"&gt;RadioNet3&lt;/a&gt;. &amp;nbsp;RadioNet3 has received funding from the European Union&amp;rsquo;s Seventh Framework Programme for research, technological development and demonstration under grant agreement no 283393.&lt;/p&gt;

&lt;p&gt;&amp;nbsp;&lt;/p&gt;

&lt;p&gt;&lt;img alt="" src="http://www.radionet-eu.org/sites/radionet-eu.org/files/cms/images/RadioNet_Logo_200.jpg" style="height:78px; width:200px" /&gt;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp; &lt;strong&gt;&lt;img alt="" src="http://www.radionet-eu.org/sites/radionet-eu.org/themes/radionet/img/header_EU.jpg" style="height:78px; width:117px" /&gt;&lt;/strong&gt;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&lt;/p&gt;
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 <name>Max-Planck-Institut für Radioastronomie, Bonn, Germany</name>
 <address>MPI für Radioastronomie 
Auf dem Hügel 69 
D-53121 Bonn
GERMANY</address>
 <room>0.02</room>
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<startDate>2015-11-30T13:00:00</startDate>
<endDate>2015-12-02T18:00:00</endDate>
<creationDate>2015-03-23T18:00:11</creationDate>
<modificationDate>2015-12-10T10:43:02</modificationDate>
<timezone>Europe/Berlin</timezone>
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 <title>Pulsar Studies with RadioAstron</title>
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   <name first="Alexey" middle="" last="Rudnitskiy"></name>
   <organization>ASC LPI</organization>
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   <name first="Alexey" middle="" last="Rudnitskiy"></name>
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   <title>Dr.</title>
   <name first="Andrey" middle="" last="Andrianov"></name>
   <organization>ASC LPI</organization>
   <emailHash>db3ebb5d33ddfac1bcce8dbb0375a5a1</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Mikhail" middle="" last="Popov"></name>
   <organization>Astro Space Center, Moscow, Russia</organization>
   <emailHash>838b4f693b554456f3df8a5e009d8ba4</emailHash>
  </user>
  <user>
   <title>Prof.</title>
   <name first="Carl" middle="" last="Gwinn"></name>
   <organization>Univ California, Santa Barbara</organization>
   <emailHash>5b5137993d2227eb16b4ce591ce05f1d</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Max-Planck-Institut für Radioastronomie, Bonn, Germany</name>
  <address>MPI für Radioastronomie 
Auf dem Hügel 69 
D-53121 Bonn
GERMANY</address>
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 </location>
 <startDate>2015-11-30T14:10:00</startDate>
 <endDate>2015-11-30T14:40:00</endDate>
 <duration>00:30</duration>
 <abstract>On behalf of the Radioastron pulsar group this report presents an overview of the studies which were done with the Radioastron space radio telescope during the first four years of mission operation, including the early and key science programs. Space-VLBI observations of pulsars with the highest angular resolution revealed the new interstellar plasma scattering effects, such as, resolving the substructure in the scattering disk. Diameters of scattering disks were measured for several pulsars and the distances to the effective scattering screens were estimated. Layers of scattering plasma were detected to be located relatively close to the Sun (10-100 pc). Such layers might be responsible for fast flux variations of compact extragalactic radio sources. A new insight on the interstellar scattering was demonstrated by study of the instantaneous visibilities which were measured with the Space-VLBI observations of giant pulses from the Crab pulsar.</abstract>
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