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The Solar Orbiter mission

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The payload consists of a suite of 8 in-situ instruments and 5 remote sensing ... EUV spectrometer, Visible-light imager/ magnetograph, coronagraph and radiometer) ... – PowerPoint PPT presentation

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Title: The Solar Orbiter mission


1
The Solar Orbiter mission
  • Solar Orbiter represents a new approach to solar
    studies.
  • A huge increase in discovery space
  • The payload consists of a suite of 8 in-situ
    instruments and 5 remote sensing instruments (EUV
    Imager, EUV spectrometer, Visible-light imager/
    magnetograph, coronagraph and radiometer)

Orbit schematic
2
(No Transcript)
3
Slow and fast solar wind
4
The solar cycle variation of the solar wind
5
The engineering challenge
  • Solar Orbiter is a specially designed three-axis
    stabilised spacecraft.
  • It is designed to always point its smallest face
    to the Sun so the spacecraft is protected by a
    sunshield.
  • At closest approach to the Sun, Solar Orbiter
    will receive 25 times the radiation per square
    metre that the Earth does.
  • The spacecraft will also be kept cool by the
    positioning of special 'radiators', which will
    dissipate excess heat into space.

6
An Imager for Solar Orbiter
The Solar Orbiter mission is a key mission for
solar system science.
  • Fundamental physical processes (waves/magnetic
    reconnection/dynamo)
  • Linking the Sun and the inner heliosphere
  • Exploring the solar atmosphere out of the
    ecliptic (slow and fast solar wind)

7
Fundamental physical processes
G-band
Ca II
  • We can, with excellent seeing, resolve 70 km in
    the photosphere with a ground-based telescope.
  • SO will allow us to do better than this even in
    the corona! (and more than an order of magnitude
    better than currently possible e.g. TRACE 750km).
  • At this resolution we will be able to observe MHD
    waves and reconnection at the fundamental
    physical scales.

Rutten et al., 2003
3-D modelling showing the interaction between
magnetic field and convection
Cattaneo, Emonet and Weiss, 2003
8
Observing up close
  • This resolution will allow us to observe magnetic
    loops at their fundamental size.
  • The smaller the scale, the more (rapid) activity
    we observe (TRACE observes with time resolution
    of seconds).

?
Factor of 100
Factor of 5
9
Linking up with in situ
10
Current Status
  • The current schedule is for the AO to be released
    in 2007 (ish).
  • Call for Letters of Intent to Propose for the
    Solar Orbiter payload in advance of the formal AO
    (this summer!).
  • The launch date is now most likely 2017 - with
    4.5 yrs to get into orbit.
  • We have been working here on technology
    development for the mission for several years -
    this will continue!
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