2017 Workshop:Ionosphere and thermosphere storm
Ionosphere and Thermosphere Response to CIR- and ICME-driven Storms
Location, Date/Time and Duration
Altitudes: MLT - Latitudes: global - Inst/Model: modeling - Other:
Format of the Workshop
Requested Specific Days
Special technology requests
The response of upper atmosphere to geomagnetic storms either driven by CIR, ICME or both is an important topic for space weather research, which is still poorly understood and not well quantified. The recent advances in theoretical simulations of the coupled magnetosphere-ionosphere-thermosphere system, data assimilation technique and new satellite mission made it possible to improve our understanding of the common and different response of the earth upper atmosphere to geomagnetic storms. It supports CEDAR Strategic Thrusts #2.
The ionosphere and thermosphere variations during geomagnetically active periods are mainly driven by energy and momentum dissipation from the magnetosphere and solar wind at high latitudes. The two major categories of interplanetary solar winds that are geoeffective are Interplanetary Coronal Mass Ejections (ICME) and Corotating Interaction Regions (CIR). ICME and CIR have distinct characteristics. ICMEs usually have a larger steady southward Bz component, whereas CIRs have highly variable Bz which fluctuates rapidly between north and south and lasts for several days. The commonality and difference in CIR- and ICME-induced thermospheric and ionospheric variations, such as their global structure, the disturbance propagation timing, and recovery, are still an open question. It is still interesting and challenging to understand how the thermosphere and ionosphere respond to the impulsive and strong driving from ICMEs and the weak or moderate, but almost constant energy dissipation for a long period of time during CIR events. We welcome presentations of both observations and numerical simulations of the storm-time changes of the thermosphere and ionosphere during ICME, CIR, and ICME+CIR storm events and the recovery of the thermosphere and ionosphere after these storms. Our session is interested in particularly recent storm events where coordinated observational campaigns have been conducted to characterize some of the key ionosphere/thermosphere parameters (such as electric fields, neutral winds and composition). These include, but not limited to, March 31-April 4, 2014; Sept 24-29, 2014; March 13-18, 2015; Sept 28-29; 2016 (all CIR storms); and March 17-19; 2013/2015 (St Patrick’ Days), and Oct 13-14, 2016 (ICME storms).
Xiaoqing Pi JPL Storm study using the Global Assimilative Ionospheric model
Wenbin Wang HAO TBD
Tony Mannucci JPL IT driving by interplanetary structures and energy budget modeling
Asti Bhatt SRI Memorial Day storm
This is where the final summary workshop report will be.
Upload presentation and link to it here. Links to other resources.
- Add links to your presentations here, including agendas, that are uploaded above. Please add bullets to separate talks. See further information on how to upload a file and link to it.