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Stas Barabash, SSPT, Kiruna

Stas Barabash, SSPT, Kiruna. Chandrayaan (Indian Moon mission). SARA = CENA + SWIM + DPU. CENA. S/C. DPU (SPL/VSSC). SWIM. SAS (IRF/ISAS/UBe). CENA (< 2kg) 0.01 ~ 3 keV ENA with mass SWIM (<0.5 kg) 0.01 ~ 15 keV Ion with mass (tuned for SW).

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Stas Barabash, SSPT, Kiruna

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  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 (< 2kg) 0.01 ~ 3 keV ENA with mass SWIM (<0.5 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. Mars Environment Analogue Platform Martin Weiser , SSPT, Kiruna 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 O+·s-1 Swedish space physics workshop. Uppsala, February 26-27, 2009

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