Stas Barabash, SSPT, Kiruna - PowerPoint PPT Presentation

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Stas Barabash, SSPT, Kiruna

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Title: Mats Holmstr m, SSPT, Kiruna Author: Mats Holmstrom Last modified by: Yamau Document presentation format: Custom Other titles: Arial AR PL ShanHeiSun Uni ... – PowerPoint PPT presentation

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Title: Stas Barabash, SSPT, Kiruna


1
Stas Barabash, SSPT, Kiruna
Chandrayaan (Indian Moon mission)
SARA CENA SWIM DPU
CENA
S/C
DPU (SPL/VSSC)
SWIM
SAS (IRF/ISAS/UBe)
CENA (lt 2kg) 0.01 3 keV ENA with mass SWIM
(lt0.5 kg) 0.01 15 keV Ion with mass (tuned for
SW)
Swedish space physics workshop. Uppsala, February
26-27, 2009
2
Stas Barabash, SSPT, Kiruna
SWIM commission data
Accelerated reflected protons
Run 1. Jan. 25
Reflected protons
Mystery!
Solar eclipse (night side)
Solar eclipse (night side)
Solar wind
Solar wind
Accelerated reflected protons
Run 2. Jan. 27
Mystery!
Solar wind
Solar eclipse (night side)
Solar eclipse (night side)
Swedish space physics workshop. Uppsala, February
26-27, 2009
3
Stas Barabash, SSPT, Kiruna
CENA commission data
Swedish space physics workshop. Uppsala, February
26-27, 2009
4
Martin Weiser , SSPT, Kiruna
Mars Environment Analogue Platform
Swedish space physics workshop. Uppsala, February
26-27, 2009
http//www.irf.se/meap-pbace
5
Futaana , SSPT, Kiruna
Phobos signature
Swedish space physics workshop. Uppsala, February
26-27, 2009
6
Mats Holmström, SSPT, Kiruna
Current Computer Modeling Projects at IRF-Kiruna
  • Uses software built on the public FLASH software
    from University of Chicago. Parallel, adaptive
    grid. Handles fluid (MHD) and particle (hybrid
    and DSMC) simulations. Uses the Akka cluster with
    5376 cores at the High Performance Computing
    Center North (HPC2N) in Umeå
  • Hybrid model of Mars-solar wind interaction under
    development.
  • Will take part in the second ISSI meeting on
    Intercomparison of Global Models and Measurements
    of the Martian Plasma Environment
  • An XMM-Newton proposal for observing Mars in
    November 2009 has been accepted. This will be the
    first time that the Mars-solar wind interaction
    is imaged in soft X-rays with simultaneous
    in-situ plasma measurements (by ASPERA-3 on Mars
    Express). With upstreams conditions known, it
    will be possible to model the X-ray production
  • Moon hybrid modeling. Will be used to interpret
    the observations of SARA on Chandrayaan-1.
  • People Mats Holmström, Shahab Fatemi (MSc, PhD
    student)?

Swedish space physics workshop. Uppsala, February
26-27, 2009
7
Sachiko Arvelius , SPT, Kiruna
Terrestrial Ion Budget
Net outflow 3 x 1025 Os-1
Swedish space physics workshop. Uppsala, February
26-27, 2009
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