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UID:128@atst.osups.universite-paris-saclay.fr
DTSTART;TZID=Asia/Tokyo;VALUE=DATE:20260802
DTEND;TZID=Asia/Tokyo;VALUE=DATE:20260808
DTSTAMP:20260112T215545Z
URL:https://atst.osups.universite-paris-saclay.fr/calendrier/aogs-2026/
SUMMARY:AOGS 2026
DESCRIPTION:From 02 to 07 August\, 2026\, a few thousand geoscientists acro
 ss diverse disciplines will gather at the 23rd annual meeting of the Asia 
 Oceania Geosciences Society at the Fukuoka International Congress Centre\,
  Japan.\n\nThe abstract submission deadline is 23 January 2026.\n\nThe ST 
 sessions and a few PS sessions are relevant to ATST. You will find below 
 a session that has been specifically advertised to ATST.\nSession PS04 —
  Aeronomy and Plasma Physics of Planetary Environments\nConveners: Dr Yuti
 an Cao (Sun Yat-sen University)\, Dr Lina Hadid (National Centre for Scien
 tific Research/Sorbonne Université-Ecole Polytechnique)\, Dr Yuki Harada 
 (Nagoya University)\, Dr Shaosui Xu (University of California\, Berkeley)\
 n\nThis session focuses on the near-space neutral and ionized environments
  of solar system objects except Earth. Thermospheres\, exospheres\, ionosp
 heres and magnetospheres are affected by the source regions at low altitud
 es and by their interaction with the solar wind. A variety of past and pre
 sent missions are dedicated to analysis of such planetary environments. Th
 is wealth of data as well as increasingly sophisticated modeling capabilit
 ies have driven great advances over the last two decades in our understand
 ing of the structure\, variability\, composition and dynamics of these env
 ironments. For example\, we are starting to elucidate the complex two-way 
 coupling between surfaces and surface-bound exospheres\, between thermosph
 eres and ionospheres\, between photochemically-dominated collisional ionos
 pheres and transport-dominated upper ionospheres\, and between all these r
 egions and the highly variable solar wind. We invite contributions concern
 ing airless bodies such as Mercury (MESSENGER\, BepiColombo)\, Earth’s m
 oon (THEMIS-ARTEMIS\, Kaguya\, Chang’e\, Chandrayaan)\, the Jovian moons
  (Galileo and Juno)\, Kuiper Belt Objects (New Horizons) and asteroids (Da
 wn) as well as bodies with substantial atmospheres such as Venus (PVO\, VE
 x\, Parker Solar Probe)\, Mars (MGS\, MEx\, MAVEN\, InSight\, EMM\, Tianwe
 n-1)\, Titan (Cassini)\, comets (Rosetta) and the giant planets (Cassini\,
  Galileo\, Juno). Both data-focused and modeling studies (and those which 
 combine the two) are encouraged. Comparative studies are particularly welc
 ome as are presentations on future missions and instrumentation concepts w
 hich address the goal of understanding and characterizing planetary near-s
 pace environments. Both solicited and contributed talks will be included.\
 n\n(Transmis par Lina Hadid)\n\n&nbsp\;
CATEGORIES:Colloques, conférences et écoles
LOCATION:Fukuoka\, Fukuoka\, Fukuoka\, Japon
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