EGU25-7438, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-7438
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 29 Apr, 15:35–15:45 (CEST)
 
Room 0.94/95
Ground state of the thermosphere and substorm time thermospheric response
Yongliang Zhang1, Qian Wu2, Jesper Gjerloev1, Larry Paxton1, and Robert Schaefer1
Yongliang Zhang et al.
  • 1The Johns Hopkins University Applied Physics Laboratory, Laurel, United States of America (yongliang.zhang@jhuapl.edu)
  • 2National Center for Atmospheric Research, Boulder, United States of America (qwu@ucar.edu)

The thermospheric composition (O/N2 ratio and NO) condition represents the state of the thermosphere. Significant changes in thermospheric composition and neutral wind are often observed during non-storm time (e.g. a weak substorm on May 29, 2023) due to continous energy and momentum input from solar wind to the geospace.  It is challenging to find days when the solar wind impact is minimized and the geospace is at its ground state (super quiet) or undisturbed conditon. After a search of SuperMAG database over two decades (2002-2022), we finally identified a few super quiet intervals with (1) AE or SME < 50 nT, SymH > 0 nT), and (2) low auroral intensities (N2 LBHS (140-150 nm) < 500 R) over 48 consecutive hours or longer. We report one super quiet interval (November 6-7, 2009) with no O/N2 depletion or NO enhancment which represents a “geopace ground state”.  

How to cite: Zhang, Y., Wu, Q., Gjerloev, J., Paxton, L., and Schaefer, R.: Ground state of the thermosphere and substorm time thermospheric response, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7438, https://doi.org/10.5194/egusphere-egu25-7438, 2025.