COSPAR20 – C3.3 – Imaging the Planets in X-rays
Soumis par mchane-y le ven, 30/08/2019 - 11:25
As someone we believe may have a scientific interest in the various topics it covers, we would like to draw your attention to a special session we are organizing at COSPAR 2020, which will be held in Sydney Australia from 15-22 August 2020, covering the broad topic of solar and stellar winds interacting with obstacles and the soft X-ray emission that results: All space science disciplines, heliophysics, planetary, and astrophysics, have an interest in understanding the complex nature of solar and stellar winds interacting with obstacles. Within recent decades, observations, modeling, and theory have shown that these interactions can be imaged in X-rays. Within our solar system, Earth, Earth’s moon, comets, Mars, Venus, Jupiter, and Pluto are known to emit X-rays resulting from their interactions with the solar wind. Furthermore, the solar wind itself emits soft X-rays when it interacts with interstellar neutrals entering the heliosphere to create a background emission for solar system objects. Similarly, stellar winds interacting with exoplanets emit soft X-rays outside our heliosphere. All these emissions are superimposed upon and must be separated from the cosmic soft X-ray background, which is itself of great interest to astrophysicists. We encourage all session submissions addressing or related to solar and/or stellar winds generating X-ray emissions. Possible topics include, but are not limited to, observations, modeling, theory, instrument concepts, and missions in both formulation and implementation, particularly the ESA/CAS SMILE mission. If you would like to participate in this session, we encourage you to submit an abstract. Note that COSPAR does not have a “one-abstract policy,” so submitting an abstract to this session will not preclude submitting another abstract on a different topic to another session. In fact, the web site for COSPAR 2020 abstract submission is open now at: https://www.cospar-assembly.org/show_infopage.php?info=52 <https://urldefense.proofpoint.com/v2/url?u=https-3A__icmsaust.us11.list-2Dmanage.com_track_click-3Fu-3Dadaae520cf9dd252446148abc-26id-3D7fcbf0238b-26e-3D05a926155b&d=DwMFaQ&c=ApwzowJNAKKw3xye91w7BE1XMRKi2LN9kiMk5Csz9Zk&r=rlSlcSGHyrpCRnPjR2mIHN20to48yTFVgfwqpEx5vGM&m=YczHDXP-Ws6rhS80kPFXoURLfi7x9FNowNHCGV3mN2c&s=QJbrDyJqa1D0for1RSYdRjehHWlSoviX8mJBfEauKmk&e=> and there is no better time than right now to submit an abstract – hope you will. Looking forward to seeing and hearing from you in Sydney next summer!! Michael, Philippe, Chi, Yoshi, and David Michael R. Collier Associate Lab Chief Geospace Laboratory Heliophysics Science Division michael.r.collier@nasa.gov 301-286-5256