Stas Barabash, SSPT, Kiruna Swedish space physics workshop. Uppsala, February 26-27, 2009 Chandrayaan (Indian Moon mission) S/C DPU (SPL/VSSC) SAS (IRF/ISAS/UBe)

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Presentation transcript:

Stas Barabash, SSPT, Kiruna Swedish space physics workshop. Uppsala, February 26-27, 2009 Chandrayaan (Indian Moon mission) S/C DPU (SPL/VSSC) SAS (IRF/ISAS/UBe) CENA SWIM CENA (< 2kg)0.01 ~ 3 keV ENA with mass SWIM (<0.5 kg)0.01 ~ 15 keV Ion with mass (tuned for SW) SARA = CENA + SWIM + DPU

Stas Barabash, SSPT, Kiruna Swedish space physics workshop. Uppsala, February 26-27, 2009 Solar eclipse (night side) Solar wind Accelerated reflected protons Mystery! Run 2. Jan. 27 Solar eclipse (night side) Solar wind Accelerated reflected protons Mystery! Solar wind Reflected protons Solar eclipse (night side) Run 1. Jan. 25 SWIM commission data

Stas Barabash, SSPT, Kiruna Swedish space physics workshop. Uppsala, February 26-27, 2009 CENA commission data

Swedish space physics workshop. Uppsala, February 26-27, 2009 Mars Environment Analogue Platform Martin Weiser, SSPT, Kiruna

Swedish space physics workshop. Uppsala, February 26-27, 2009 Futaana, SSPT, Kiruna Phobos signature

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)‏ Mats Holmström, SSPT, Kiruna Swedish space physics workshop. Uppsala, February 26-27, 2009

Sachiko Arvelius, SPT, Kiruna Terrestrial Ion Budget Net outflow 3 x O + ·s -1