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UPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. ORBIT VISUALIZATION TOOL 3.0 USER GUIDE Orbit Visualization Tool (OVT) User Guide. The magnetic field models include standard internal field model IGRF 1950-2000 and Tsyganenko models of the external magnetospheric field: T87, T89, T96 and T2001.; The bow shock model is according to Farris et al, GRL, v. 18, p.1821, 1991, and Cairns et al., JGR, v.100, p.47, 1995 ; The magnetopause model is according to Shue et al., JGR, v. 103, SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen) SOLUTION - SPACE.IRFU.SE Solution to Exam in Antenna Theory Time: 17 March 2009, at 8.00–13.00. Location: Gimogatan 4, Sal 2 You may bring: Laboratory reports, pocket calculator, English dictionary, Råde-Westergren:“Beta”,
UPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. ORBIT VISUALIZATION TOOL 3.0 USER GUIDE Orbit Visualization Tool (OVT) User Guide. The magnetic field models include standard internal field model IGRF 1950-2000 and Tsyganenko models of the external magnetospheric field: T87, T89, T96 and T2001.; The bow shock model is according to Farris et al, GRL, v. 18, p.1821, 1991, and Cairns et al., JGR, v.100, p.47, 1995 ; The magnetopause model is according to Shue et al., JGR, v. 103, SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen) SOLUTION - SPACE.IRFU.SE Solution to Exam in Antenna Theory Time: 17 March 2009, at 8.00–13.00. Location: Gimogatan 4, Sal 2 You may bring: Laboratory reports, pocket calculator, English dictionary, Råde-Westergren:“Beta”,
UPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Previous projects. PhD and licentiate (FL) projects by year completed (since 2002). Major research project and supervisor initials in brackets. 2021. Fredrik Johansson, Rosetta Observations of Plasma and Dust at Comet 67P 2019. Andeas Johlander, Ion dynamics and structure of collisionless shocks in space ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Master Projects, BSc projects, Project course projects, Examensarbeten, Kandidatprojekt etc. While we have hosted project students from many universities in- and outside Sweden, Uppsala university students dominate, for obvious reasons. Most student projects are 30 credits (30 hp), corresponding to roughly 20 weeks of full time work, but 15 or ANDERS ERIKSSON , PHD, SCIENTIST http://www.space.irfu.se/aie/index.html last modified onFriday, 15-Sep-2017 18:47:51 CEST SOLUTION - SPACE.IRFU.SE Solution to Exam in Antenna Theory Time: 17 March 2009, at 8.00–13.00. Location: Gimogatan 4, Sal 2 You may bring: Laboratory reports, pocket calculator, English dictionary, Råde-Westergren:“Beta”,
SOLUTION TO EXAM IN ANTENNA THEORY WESTERGREN: “BETA Solution to Exam in Antenna Theory Time: 18 March 2010, at 8.00–13.00. Location: Polacksbacken, Skrivsal You may bring: Laboratory reports, pocket calculator, English dictionary, Råde- PLASMA PARAMETERS FROM THE ROSETTA LAP INSTRUMENT 2 Abstract The focus of this thesis is the extraction of plasma parameters using the Lang-muir probes mounted on the Rosetta spacecraft. These probes, developed by theUPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
CLUSTER: ELECTRIC FIELD AND WAVE EXPERIMENT (EFW) The Electric Field and Wave (EFW) instrument with Mats André as Principal Investigator is designed to measure the electric field and density variations. The instrument includes two pairs of probes on wire booms in the spin plane, each with a probe-to-probe separation of 88 m. Typically EFW measures electric fields at 25 or 450 samples persecond.
ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. PHASES OF AN ESA HARDWARE PROJECT EXPLAINED •A good JUICE requirement: The PI shall ensure that the unit identification code is composed of the following threeparts: •3 to 4 characters for instrument identification, (e.g. RPWI) •3 characters for unit identification, (e.g. Digital Processing Unit, DPU) •2 characters for model identification ( ST for Structural Thermal Model, EM for Engineering Model, QM for Qualification Model SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen)UPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
CLUSTER: ELECTRIC FIELD AND WAVE EXPERIMENT (EFW) The Electric Field and Wave (EFW) instrument with Mats André as Principal Investigator is designed to measure the electric field and density variations. The instrument includes two pairs of probes on wire booms in the spin plane, each with a probe-to-probe separation of 88 m. Typically EFW measures electric fields at 25 or 450 samples persecond.
ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. PHASES OF AN ESA HARDWARE PROJECT EXPLAINED •A good JUICE requirement: The PI shall ensure that the unit identification code is composed of the following threeparts: •3 to 4 characters for instrument identification, (e.g. RPWI) •3 characters for unit identification, (e.g. Digital Processing Unit, DPU) •2 characters for model identification ( ST for Structural Thermal Model, EM for Engineering Model, QM for Qualification Model SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen) ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Previous projects. PhD and licentiate (FL) projects by year completed (since 2002). Major research project and supervisor initials in brackets. 2021. Fredrik Johansson, Rosetta Observations of Plasma and Dust at Comet 67P 2019. Andeas Johlander, Ion dynamics and structure of collisionless shocks in space ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. ANDERS ERIKSSON , PHD, SCIENTIST http://www.space.irfu.se/aie/index.html last modified onFriday, 15-Sep-2017 18:47:51 CEST ORBIT VISUALIZATION TOOL : WHAT IS OVT Orbit Visualization Tool (OVT) is a software designed for interactive 3D visualization of saltellite orbits and scientific data ORBIT VISUALIZATION TOOL 3.0 USER GUIDE Orbit Visualization Tool (OVT) User Guide. The magnetic field models include standard internal field model IGRF 1950-2000 and Tsyganenko models of the external magnetospheric field: T87, T89, T96 and T2001.; The bow shock model is according to Farris et al, GRL, v. 18, p.1821, 1991, and Cairns et al., JGR, v.100, p.47, 1995 ; The magnetopause model is according to Shue et al., JGR, v. 103, SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Master Projects, BSc projects, Project course projects, Examensarbeten, Kandidatprojekt etc. While we have hosted project students from many universities in- and outside Sweden, Uppsala university students dominate, for obvious reasons. Most student projects are 30 credits (30 hp), corresponding to roughly 20 weeks of full time work, but 15 or MISSION DESIGN AND SYSTEMS ENGINEERING FOR SPACECRAFT System Engineering: Need to examine the system and processes as a whole Engineering process is iterative, not linear Orbits: Elliptic orbits are perturbed by small forces Velocity change ΔV is the fundamental parameter when changing orbits Launchers Many available launchers to choose from, but not many inexpensive ones Ground Support: Communications link is vital for command and control, as SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen)WWW.SPACE.IRFU.SE
Created Date: 2/19/2005 11:20:33 AMUPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
CLUSTER: ELECTRIC FIELD AND WAVE EXPERIMENT (EFW) The Electric Field and Wave (EFW) instrument with Mats André as Principal Investigator is designed to measure the electric field and density variations. The instrument includes two pairs of probes on wire booms in the spin plane, each with a probe-to-probe separation of 88 m. Typically EFW measures electric fields at 25 or 450 samples persecond.
ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. PHASES OF AN ESA HARDWARE PROJECT EXPLAINED •A good JUICE requirement: The PI shall ensure that the unit identification code is composed of the following threeparts: •3 to 4 characters for instrument identification, (e.g. RPWI) •3 characters for unit identification, (e.g. Digital Processing Unit, DPU) •2 characters for model identification ( ST for Structural Thermal Model, EM for Engineering Model, QM for Qualification Model SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen)UPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
CLUSTER: ELECTRIC FIELD AND WAVE EXPERIMENT (EFW) The Electric Field and Wave (EFW) instrument with Mats André as Principal Investigator is designed to measure the electric field and density variations. The instrument includes two pairs of probes on wire booms in the spin plane, each with a probe-to-probe separation of 88 m. Typically EFW measures electric fields at 25 or 450 samples persecond.
ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. PHASES OF AN ESA HARDWARE PROJECT EXPLAINED •A good JUICE requirement: The PI shall ensure that the unit identification code is composed of the following threeparts: •3 to 4 characters for instrument identification, (e.g. RPWI) •3 characters for unit identification, (e.g. Digital Processing Unit, DPU) •2 characters for model identification ( ST for Structural Thermal Model, EM for Engineering Model, QM for Qualification Model SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen) ÅNGSTRÖM - IRFU.SE The Ångström Laboratory(1) is located at Polacksbacken, about 2 km south of the center of Uppsala, close to Dag Hammarskjölds väg, MIC and BMC.. By bus - For more details, see UL website. SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Previous projects. PhD and licentiate (FL) projects by year completed (since 2002). Major research project and supervisor initials in brackets. 2021. Fredrik Johansson, Rosetta Observations of Plasma and Dust at Comet 67P 2019. Andeas Johlander, Ion dynamics and structure of collisionless shocks in space ORBIT VISUALIZATION TOOL : HOME The Orbit Visualization Tool (OVT) is a software for visualization of satellite orbits in the Earth's magnetic field. The program can display satellite orbits in five coordinate systems ( GEI, GEO, GSM, SMC, GSE ), satellite footprints projected on the Earth's surface and shown in either geographic (GEO) or geomagnetic (SMC) coordinates. ANDERS ERIKSSON , PHD, SCIENTIST http://www.space.irfu.se/aie/index.html last modified onFriday, 15-Sep-2017 18:47:51 CEST ORBIT VISUALIZATION TOOL : WHAT IS OVT Orbit Visualization Tool (OVT) is a software designed for interactive 3D visualization of saltellite orbits and scientific data ORBIT VISUALIZATION TOOL 3.0 USER GUIDE Orbit Visualization Tool (OVT) User Guide. The magnetic field models include standard internal field model IGRF 1950-2000 and Tsyganenko models of the external magnetospheric field: T87, T89, T96 and T2001.; The bow shock model is according to Farris et al, GRL, v. 18, p.1821, 1991, and Cairns et al., JGR, v.100, p.47, 1995 ; The magnetopause model is according to Shue et al., JGR, v. 103, SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Master Projects, BSc projects, Project course projects, Examensarbeten, Kandidatprojekt etc. While we have hosted project students from many universities in- and outside Sweden, Uppsala university students dominate, for obvious reasons. Most student projects are 30 credits (30 hp), corresponding to roughly 20 weeks of full time work, but 15 or MISSION DESIGN AND SYSTEMS ENGINEERING FOR SPACECRAFT System Engineering: Need to examine the system and processes as a whole Engineering process is iterative, not linear Orbits: Elliptic orbits are perturbed by small forces Velocity change ΔV is the fundamental parameter when changing orbits Launchers Many available launchers to choose from, but not many inexpensive ones Ground Support: Communications link is vital for command and control, as SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen)WWW.SPACE.IRFU.SE
Created Date: 2/19/2005 11:20:33 AMUPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
ANDERS ERIKSSON , PHD, SCIENTIST http://www.space.irfu.se/aie/index.html last modified onFriday, 15-Sep-2017 18:47:51 CEST MISSION DESIGN AND SYSTEMS ENGINEERING FOR SPACECRAFT System Engineering: Need to examine the system and processes as a whole Engineering process is iterative, not linear Orbits: Elliptic orbits are perturbed by small forces Velocity change ΔV is the fundamental parameter when changing orbits Launchers Many available launchers to choose from, but not many inexpensive ones Ground Support: Communications link is vital for command and control, as PHASES OF AN ESA HARDWARE PROJECT EXPLAINED •A good JUICE requirement: The PI shall ensure that the unit identification code is composed of the following threeparts: •3 to 4 characters for instrument identification, (e.g. RPWI) •3 characters for unit identification, (e.g. Digital Processing Unit, DPU) •2 characters for model identification ( ST for Structural Thermal Model, EM for Engineering Model, QM for Qualification ModelOPENPROJECT
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SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen)UPPSALA
Swedish Institute of Space Physics webpages. Last update: 2021-04-16 /Jan Karlsson2021-04-16 /Jan Karlsson SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA 15 Jan 2021: At 13:15 on Zoom, Fredrik Leffe Johansson defended his PhD thesis Rosetta Observations of Plasma and Dust at Comet 67P.Faculty opponent was Dr. Nicolas André, IRAP, Toulouse. Check out this summary (scroll down for English).. 21 Dec 2020: The ESA Planetary Science Archive has now released the full and complete set of data from LAP, our Langmuir probe instrument on the SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Our Courses in Space Physics. at Uppsala University. Space Physics / Rymdfysik (1FA255, 5 hp) Masters course in period 1. Plasma Waves (8 hp) PhD course given during fall 2020. Magnetic Reconnection (10 hp) PhD course given during spring 2020. Electronics in Extreme Environments / Elektronik i extrema miljöer (1FA259, 5 hp) SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Since then, have have used our Langmuir probe instrument onboard for investigating the space physics of the Saturn system, including its rings and moons, particularly Titan and Enceladus. The Langmuir probe is designed and built by us at the Swedish Institute of Space Physics in Uppsala, and we get a lot of nice data and results. probe overTitan.
ANDERS ERIKSSON , PHD, SCIENTIST http://www.space.irfu.se/aie/index.html last modified onFriday, 15-Sep-2017 18:47:51 CEST MISSION DESIGN AND SYSTEMS ENGINEERING FOR SPACECRAFT System Engineering: Need to examine the system and processes as a whole Engineering process is iterative, not linear Orbits: Elliptic orbits are perturbed by small forces Velocity change ΔV is the fundamental parameter when changing orbits Launchers Many available launchers to choose from, but not many inexpensive ones Ground Support: Communications link is vital for command and control, as PHASES OF AN ESA HARDWARE PROJECT EXPLAINED •A good JUICE requirement: The PI shall ensure that the unit identification code is composed of the following threeparts: •3 to 4 characters for instrument identification, (e.g. RPWI) •3 characters for unit identification, (e.g. Digital Processing Unit, DPU) •2 characters for model identification ( ST for Structural Thermal Model, EM for Engineering Model, QM for Qualification ModelOPENPROJECT
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SPACE PHYSICS LECTURE NOTES Space Physics Lecture Notes From the Course flRymdfysik Ifl Anders I. Eriksson Department of Astronomy and Space Physics Uppsala University October 2002 SPACE PROJECT MANAGEMENT Space Project Management Chris Cully 8 April 2008. chris@irfu.se (Based on 2007 lectures by Petrus Hyvönen) SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Previous projects. PhD and licentiate (FL) projects by year completed (since 2002). Major research project and supervisor initials in brackets. 2021. Fredrik Johansson, Rosetta Observations of Plasma and Dust at Comet 67P 2019. Andeas Johlander, Ion dynamics and structure of collisionless shocks in space ANDERS ERIKSSON , PHD, SCIENTIST http://www.space.irfu.se/aie/index.html last modified onFriday, 15-Sep-2017 18:47:51 CEST CLUSTER: ELECTRIC FIELD AND WAVE EXPERIMENT (EFW) The Electric Field and Wave (EFW) instrument with Mats André as Principal Investigator is designed to measure the electric field and density variations. The instrument includes two pairs of probes on wire booms in the spin plane, each with a probe-to-probe separation of 88 m. Typically EFW measures electric fields at 25 or 450 samples persecond.
SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Master Projects, BSc projects, Project course projects, Examensarbeten, Kandidatprojekt etc. While we have hosted project students from many universities in- and outside Sweden, Uppsala university students dominate, for obvious reasons. Most student projects are 30 credits (30 hp), corresponding to roughly 20 weeks of full time work, but 15 orOPENPROJECT
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ORBIT VISUALIZATION TOOL 3.0 USER GUIDE Orbit Visualization Tool (OVT) User Guide. The magnetic field models include standard internal field model IGRF 1950-2000 and Tsyganenko models of the external magnetospheric field: T87, T89, T96 and T2001.; The bow shock model is according to Farris et al, GRL, v. 18, p.1821, 1991, and Cairns et al., JGR, v.100, p.47, 1995 ; The magnetopause model is according to Shue et al., JGR, v. 103, SPACE MISSION DESIGN Space Mission Design Project Course code: 1RF109 Teachers: Mats André, ma@irfu.se, Å84107, 018-4715913 Chris Cully, chris@irfu.se, Å84113, 076-2528347 ORBIT VISUALIZATION TOOL : WHAT IS OVT Orbit Visualization Tool (OVT) is a software designed for interactive 3D visualization of saltellite orbits and scientific data SWEDISH INSTITUTE OF SPACE PHYSICS, UPPSALA Student Project (30 c)/Examensarbete (30 hp) Reconstructing ICMEs with the toroidal Grad-Shafranov method Student: Moa Skan, Uppsala University Supervisor: Emiliya Yordanova WAKE FORMATION BY ION SCATTERING ON A POSITIVELY CHARGED 2 FIG. 1: Illustration of wake formation when the ion energy is above (a) or below (b) the equivalent spacecraft potential. where T i is the ion temperature, the ions scatter on the electrostatic potential structure around the spacecraft rather than reaching the solidobstacle itself.
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Swedish Institute of Space Physics , Uppsala, is integrated with the Department of Physics and Astronomy of the Uppsala University and located at the Ångström Laboratory. -------------------------GENERAL INFO
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