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X-WR-CALDESC:Events for eSpace - EPFL Space Center
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BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20240222T171500
DTEND;TZID=Europe/Zurich:20240222T181500
DTSTAMP:20240223T141511Z
CREATED:20240219T150302Z
LAST-MODIFIED:20240223T141511Z
UID:15619-1708622100-1708625700@espace.epfl.ch
SUMMARY:Solar Flare X-ray Observations with a Cubesat
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/solar-flares-cubesat/
LOCATION:ZOOM
CATEGORIES:Conference,eSpace Seminars
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2024/02/espace-seminar-krucker.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20240124T161500
DTEND;TZID=Europe/Zurich:20240124T171500
DTSTAMP:20240111T132356Z
CREATED:20240111T131850Z
LAST-MODIFIED:20240111T132356Z
UID:15578-1706112900-1706116500@espace.epfl.ch
SUMMARY:USSF-MIT researchers present their work : AI Technologies and simulation tools for SSA - Space Sustainability and Policy
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/ussf-space-sustainability-policy/
LOCATION:ZOOM
CATEGORIES:Conference,eSpace Seminars
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2024/01/espace-seminar-USSF.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20231128T173000
DTEND;TZID=Europe/Zurich:20231128T183000
DTSTAMP:20231115T095831Z
CREATED:20231115T082925Z
LAST-MODIFIED:20231115T095831Z
UID:15418-1701192600-1701196200@espace.epfl.ch
SUMMARY:The European Aerospace Sector: Perspectives from the industry\, academia and the public sector
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/spanish-delegation-epfl/
LOCATION:EPFL Campus room SV 1717
CATEGORIES:Conference,eSpace Seminars
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2023/11/espace-seminar_spain.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20231113T173000
DTEND;TZID=Europe/Zurich:20231113T183000
DTSTAMP:20231106T154251Z
CREATED:20231106T103826Z
LAST-MODIFIED:20231106T154251Z
UID:15326-1699896600-1699900200@espace.epfl.ch
SUMMARY:What can we do about climate change?
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/charling-tao/
LOCATION:EPFL Campus room MED 0 1418
CATEGORIES:Conference,eSpace Seminars
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2023/11/espace-seminar_TAO_website.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20231011T173000
DTEND;TZID=Europe/Zurich:20231011T183000
DTSTAMP:20231110T110824Z
CREATED:20230928T125027Z
LAST-MODIFIED:20231110T110824Z
UID:15152-1697045400-1697049000@espace.epfl.ch
SUMMARY:SWIR/NIR SPAD Image Sensors for LIDAR  and Quantum Imaging Applications\, by prof. Edoardo Charbon
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/swir-nir-spadedoardo-charbon/
LOCATION:ZOOM
CATEGORIES:Conference,eSpace Seminars,Webinar
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2023/09/espace-seminar-edoardo.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20230927T173000
DTEND;TZID=Europe/Zurich:20230927T183000
DTSTAMP:20230907T134758Z
CREATED:20230907T110700Z
LAST-MODIFIED:20230907T134758Z
UID:14987-1695835800-1695839400@espace.epfl.ch
SUMMARY:RF System Design for Robotic Spacecraft Requirements - Design Challenges and Emerging Technologies\, by Hannes Bartle
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/ref-system-bartle/
LOCATION:ZOOM
CATEGORIES:Conference,eSpace Seminars,Webinar
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2023/09/bartle-27.09.2023.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20230522T170000
DTEND;TZID=Europe/Zurich:20230522T180000
DTSTAMP:20230516T092839Z
CREATED:20230516T092839Z
LAST-MODIFIED:20230516T092839Z
UID:14491-1684774800-1684778400@espace.epfl.ch
SUMMARY:ESA’s ambition for space in Europe\, by Simona Richard
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/esa-in-europe/
LOCATION:ZOOM
CATEGORIES:eSpace Seminars,Webinar
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2023/05/Headshot_SR.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20230313T163000
DTEND;TZID=Europe/Zurich:20230313T173000
DTSTAMP:20230314T170707Z
CREATED:20230306T163248Z
LAST-MODIFIED:20230314T170707Z
UID:13781-1678725000-1678728600@espace.epfl.ch
SUMMARY:Sustainable Space Hub: new technologies and services to secure the long-term usability of space
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/sustainable-space-hub/
LOCATION:ZOOM
CATEGORIES:eSpace Seminars,Webinar
ATTACH;FMTTYPE=image/png:https://espace.epfl.ch/wp-content/uploads/2023/03/Logo-Complet-fond-clair-couleur.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20221212T160000
DTEND;TZID=Europe/Zurich:20221212T170000
DTSTAMP:20221213T124753Z
CREATED:20221123T133805Z
LAST-MODIFIED:20221213T124753Z
UID:13377-1670860800-1670864400@espace.epfl.ch
SUMMARY:Lunar Hub: a venture to explore the extreme and the uncharted\, by David Rodríguez
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/lunarhub/
LOCATION:ZOOM
CATEGORIES:eSpace Seminars
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2021/10/lunar-banner.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20221114T160000
DTEND;TZID=Europe/Zurich:20221114T170000
DTSTAMP:20221125T095242Z
CREATED:20220912T140202Z
LAST-MODIFIED:20221125T095242Z
UID:12880-1668441600-1668445200@espace.epfl.ch
SUMMARY:Solar System Objects (SSOs) Pipeline for the Euclid Mission\, by Aurelien Verdier
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/solar-system-objects/
LOCATION:ZOOM
CATEGORIES:eSpace Seminars
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2022/09/20220910_1348512.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20221107T171500
DTEND;TZID=Europe/Zurich:20221107T181500
DTSTAMP:20221125T095121Z
CREATED:20221025T090415Z
LAST-MODIFIED:20221125T095121Z
UID:13147-1667841300-1667844900@espace.epfl.ch
SUMMARY:VIRUP: The Virtual Reality Universe Project\, by Yves Revaz & Florian Cabot
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/virup-the-virtual-reality-universe-project/
LOCATION:ZOOM
CATEGORIES:eSpace Seminars
ATTACH;FMTTYPE=image/png:https://espace.epfl.ch/wp-content/uploads/2022/10/galaxy.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Zurich:20221003T170000
DTEND;TZID=Europe/Zurich:20221003T180000
DTSTAMP:20221021T104530Z
CREATED:20220912T125353Z
LAST-MODIFIED:20221021T104530Z
UID:12865-1664816400-1664820000@espace.epfl.ch
SUMMARY:ExoMars: a planetary mission to explore Mars\, by Francesco Garrone
DESCRIPTION:The X-ray imaging spectrometer STIX onboard ESA’s flagship mission Solar Orbiter was designed and build with a Swiss lead at the University of Applied Sciences Northwestern Switzerland (FHNW). STIX is now in its fourth year of operation and has recorded so far over 45’000 solar flares. The STIX detectors designed by CEA\, France\, work extremely reliably with all 32 detectors still working nominally showing only minimal degradation due to radiation damage. We still have over 50 STIX flight spare detectors available\, and four of those will fly on a NASA cubesat mission called PADRE lead by UC Berkeley (PI J.C. Martinez-Oliveros). In this talk\, Säm Krucker will introduce the science of solar flares and the STIX instrument and then show how STIX X-ray detectors are used in the PADRE cubsat mission. \nSäm Krucker's main scientific interests are in problems of plasma astrophysics\, especially solar and heliospheric physics\, from an observational and experimental point of view. He has a strong background in space hardware and I have been the PI of NASA’s Small Explorer mission RHESSI and NASA’s sounding rocket program FOXSI. He is currently the lead of the hard X-ray imaging spectrometer STIX onboard ESA’s Solar Orbiter mission.
URL:https://espace.epfl.ch/event/exomars-a-planetary-mission-to-explore-mars/
LOCATION:ZOOM
CATEGORIES:eSpace Seminars
ATTACH;FMTTYPE=image/jpeg:https://espace.epfl.ch/wp-content/uploads/2022/09/IMG_65442.jpg
END:VEVENT
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