[IGPP Everyone] SPACE PHYSICS SEMINAR Winter Quarter Schedule - Friday January 8th - 3:30pm - STORM: Science Objectives and Mission Design (D. Sibeck, NASA GSFC)

Emmanuel V. Masongsong emasongsong at igpp.ucla.edu
Mon Jan 4 13:38:34 PST 2021



Dear all, 




The list of speakers for the Winter Quarter seminars is below. Given the many exciting Heliophysics missions under development and the move by NASA/HQ to actively shape the future of the field through white papers and a special Heliophysics 2050 workshop on May 3-5, 2021, the flavor of the Seminar series will be dominated by the science of new Heliophysics missions. 





***Students please enroll for seminar in: AOS M275B or EPSS M288B and for Journal Club in: EPSS 293B*** 




Preliminary list of speakers: 

Date Seminar Speaker Topic: 

January 8, 2021 David Sibeck, GSFC STORM Science Objectives and Mission Design (Zoom+talk details below) 

January 15, 2021 Xu Zhang, UCLA [TBC] Plasma sheet waves 

January 22, 2021 Sheng Tian [U Minn.] Dipolarization propagation 

January 29, 2021 Kristina Lynch ARCS 

February 5, 2021 Bart De Pontieu MUSE 

February 12, 2021 Craig DeForest PUNCH 

February 19, 2021 Lara Waldrop GLIDE 

February 26, 2021 TBC TBC 

March 5, 2021 Craig Kletzing, Uiowa TRACERS 

March 12, 2021 Don Hassler, SwRI [TBC]Solaris 



Best wishes 



Vassilis 

SPACE PHYSICS SEMINAR 




DEPARTMENT OF EARTH, PLANETARY, AND SPACE SCIENCES 

DEPARTMENT OF ATMOSPHERIC AND OCEANIC SCIENCES 

UNIVERSITY OF CALIFORNIA, LOS ANGELES 




ZOOM Link: https://ucla.zoom.us/j/94454128469?pwd=Qm9OSmZZekN5S0RoVTFITEs0N296QT09 

Meeting ID: 944 5412 8469 Passcode: 263337 



STORM: Science Objectives and Mission Design 

David Sibeck, NASA GSFC 

STORM will provide the first-ever global view of the Sun-Earth system. STORM takes simultaneous observations of the solar wind and the response of Earth's magnetosphere, including the magnetopause, auroral oval, and ring current dynamics, using global multispectral and neutral atom imaging to quantify the global circulation of the energy that powers space weather. STORM employs a single lunar swing-by to enter a circular 90deg inclination orbit with a radius of 30RE and a period of 9.65 days which precesses a full 360deg a year. This orbit enables observations of the magnetosphere's response to varying solar wind conditions from the full range of vantage points over time scales encompassing all space weather phenomena. Furthermore, this orbit allows scientific return 100% of the time from at least as ingle instrument and up to 83% of the time from all instruments, allowing for extended observation periods. STORM's two in-situ instruments, the magnetometer and ion electron spectrometer, measure the local magnetic field and plasma. STORM's 4 imagers, the soft x-ray imager (XRI), far ultraviolet imager (FUV) and energetic neutral atom imager (ENA), and LAICA, make nearly continuous observations of the magnetopause and bow shock, the auroral oval, the Earth's ring current, and the exosphere, respectively. 



Friday, January 8, 2021 

3:30 - 5:00 PM 




In-Charge: Vassilis Angelopoulos 
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