A scheme for forecasting severe space weather

Author(s):  
Balan Nanan

<p>We have developed and tested a scheme for forecasting severe space weather (SvSW) that caused all known electric power outages and telecommunication system failures since 1957 and the Carrington event of 1859. The SvSW events of 04 August 1972 has puzzled the scientific community as it occurred during a moderate storm (DstMin = -124 nT) while all other SvSW events occurred during super storms (DstMin ≤ -250 nT). The solar wind velocity V and IMF Bz measured by ACE satellite at the L1 point since 1998 are used. For the earlier SvSW events such as the Carrington event of 1859, Quebec event of 1989, and the events in February 1958 and August 1972 we used the information from the literature. The coincidence of high ICME front (or shock) velocity ΔV (sudden increase in V over the background by over 275 km/s) and sufficiently large Bz southward at the time of the ΔV increase is associated with SvSW; and their product (ΔV×Bz) is found to exhibit a large negative spike at the speed increase. Such a product (ΔV×Bz) exceeding a threshold seems suitable for forecasting SvSW, with a maximum forecasting time of 35 minutes using ACE data. However, the coincidence of high V (not containing ΔV) and large Bz southward does not correspond to SvSW, indicating the importance of the impulsive action of high ΔV and large Bz southward coming through when they coincide. The need for the coincidence is verified using the CRCM.</p>

2020 ◽  
Author(s):  
Hua-Shan Shi ◽  
Zheng-Xian Chen ◽  
Wing-Huen Ip

<p>A number of moon-sized objects in the solar system are characterized by the formation of a surface-bound exosphere. These include the Moon, Ceres, Jupiter’s icy moons, namely, Europa, Ganymede and Callisto, and several of the Saturnian icy moons including Rhea, Dione, and Tethys. There are several major source mechanisms ranging from micrometeoroid bombardment, photo-stimulated desorption, and energetic ion sputtering - in addition to the surface (or subsurface) thermal sublimation in the case of Ceres and the icy Moon. It is interesting that Ceres and the Moon could experience extreme space weather effects when they encounter large solar flare events or coronal mass ejection events. An important consequence is the production of a transient exosphere due to the sudden increase of ion sputtering rates. We have developed time-dependent Monte Carlo models that can be applied to the Moon and Ceres. Some simulation results will be described in this presentation with a view to construct the CME-driven H<sub>2</sub>O and O<sub>2</sub> exosphere of Ceres and the flare-up of the lunar sodium corona and tail emission.</p>


2019 ◽  
Vol 9 ◽  
pp. A34 ◽  
Author(s):  
Alexa J. Halford ◽  
Adam C. Kellerman ◽  
Katherine Garcia-Sage ◽  
Jeffrey Klenzing ◽  
Brett A. Carter ◽  
...  

The space physics community continues to grow and become both more interdisciplinary and more intertwined with commercial and government operations. This has created a need for a framework to easily identify what projects can be used for specific applications and how close the tool is to routine autonomous or on-demand implementation and operation. We propose the Application Usability Level (AUL) framework and publicizing AULs to help the community quantify the progress of successful applications, metrics, and validation efforts. This framework will also aid the scientific community by supplying the type of information needed to build off of previously published work and publicizing the applications and requirements needed by the user communities. In this paper, we define the AUL framework, outline the milestones required for progression to higher AULs, and provide example projects utilizing the AUL framework. This work has been completed as part of the activities of the Assessment of Understanding and Quantifying Progress working group which is part of the International Forum for Space Weather Capabilities Assessment.


1999 ◽  
Vol 1 ◽  
pp. S17-S17
Author(s):  
A FERNANDES ◽  
E DIAS ◽  
M FIUZA ◽  
I DIONISIO ◽  
F VEIGA ◽  
...  

Space Weather ◽  
2004 ◽  
Vol 2 (4) ◽  
pp. n/a-n/a ◽  
Author(s):  
Anna Belehaki ◽  
Jean Lilensten ◽  
Toby Clark
Keyword(s):  

Space Weather ◽  
2003 ◽  
Vol 1 (1) ◽  
pp. n/a-n/a ◽  
Author(s):  
Robert Robinson
Keyword(s):  

Space Weather ◽  
2005 ◽  
Vol 3 (1) ◽  
pp. n/a-n/a
Author(s):  
Sarah Simpson
Keyword(s):  

Space Weather ◽  
2004 ◽  
Vol 2 (12) ◽  
pp. n/a-n/a
Author(s):  
Jonathan Lifland
Keyword(s):  

Space Weather ◽  
2004 ◽  
Vol 2 (7) ◽  
pp. n/a-n/a
Author(s):  
Sarah Simpson
Keyword(s):  

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