BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Instituto de Astrofísica de Andalucía - ECPv6.15.20//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Instituto de Astrofísica de Andalucía
X-ORIGINAL-URL:https://www.iaa.csic.es
X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Paris
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20230326T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20231029T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20240331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20241027T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20250330T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20251026T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240924T123000
DTEND;TZID=Europe/Paris:20240924T133000
DTSTAMP:20260423T164827
CREATED:20240924T074925Z
LAST-MODIFIED:20250125T200955Z
UID:21952-1727181000-1727184600@www.iaa.csic.es
SUMMARY:Constraining the Meteoroid Flux in the inner solar system
DESCRIPTION:​The inner solar system is populated by Interplanetary Dust Particles (IDPs) released from cometary trails and collisions between asteroids. Planetary bodies and satellites therefore encounter a cloud of IDPs along their orbits\, giving rise to a permanent bombardment on their respective atmospheres or surfaces. Constraining the magnitude of the mass influx of IDPs onto a solar system body is crucial for understanding the effects in their atmospheres and on their surfaces. \nFor planetary bodies with atmospheres\, collisions with air molecules lead to the thermal ablation of IDPs above their melting temperature and\, therefore\, their constituent elements evaporate and produce layers of free neutral and ionized atoms\, being Mg\, Fe\, Si\, and Na the major metallic species. Metallic layers in the Earth’s atmosphere have been widely studied for decades using ground-based lidar and space-based optical spectroscopy. In the case of Mars\, the Mars Atmosphere and Volatile Evolution (MAVEN) Imaging Ultraviolet Spectrograph (IUVS) reported the first detection of a persistent Mg+ layer in Mars’ atmosphere peaking around 90 km. \nIn this talk\, firstly I will review the most relevant modelling results for the meteoroid mass influx at the Earth\, Mars\, and Venus. Second\, I will discuss the results of the most recent state-of-the-art models able to provide a comprehensive description of the meteoroid impacts accounting for the temporal\, latitudinal\, and seasonal distributions of the main meteoroid populations in the inner solar system. \nFecha: 24/09/2024 – 12:30Conferenciante: Dr. Juan Diego Carrillo SánchezFiliación: NASA Goddard\, US
URL:https://www.iaa.csic.es/evento/constraining-the-meteoroid-flux-in-the-inner-solar-system/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
END:VCALENDAR