skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Role of IMF B y in the prompt electric field disturbances over equatorial ionosphere during a space weather event

Abstract

On 7 January 2005 (Ap=40) prompt penetration electric field perturbations of opposite polarities were observed over Thumba and Jicamarca on a few occasions during 13:45–16:30 UT. However, the electric field was found to be eastward during 14:45–15:30 UT over both Thumba and Jicamarca contrary to the general expectation wherein opposite polarities are expected at nearly antipodal points. On closer scrutiny, three important observational features are noticed during 14:10–15:15 UT. First, during 14:10–14:45 UT, despite increasing southward interplanetary magnetic field (IMF) B z condition, the already westward electric field over Thumba weakened (less westward) while the eastward electric field over Jicamarca intensified (more eastward). Second, the electric field not only became anomalously eastward over Thumba but also got intensified further during 14:45–15:00 UT similar to Jicamarca. Third, during 15:00–15:15 UT, despite IMF B z remaining steadily southward, the eastward electric field continued to intensify over Thumba but weakened over Jicamarca. It is suggested that the changes in IMF B y component under southward IMF B z condition are responsible for skewing the ionospheric equipotential patterns over the dip equator in such a way that Thumba came into the same DP2 cell as that of Jicamarca leading to anomalous electric field variations.more » Magnetic field measurements along the Indian and Jicamarca longitude sectors and changes in high-latitude ionospheric convection patterns provide credence to this proposition. Therefore, in conclusion, the present investigation shows that the variations in IMF B y are fundamentally important to understand the prompt penetration effects over low latitudes.« less

Authors:
ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [4]
  1. Physical Research Lab., Ahmedabad (India)
  2. Indian Inst. of Geomagnetism, Navi Mumbai (India)
  3. Los Alamos National Lab. (LANL), Los Alamos, NM (United States); New Mexico Consortium, Los Alamos, NM (United States)
  4. Virginia Polytechnic Inst. and State Univ. (Virginia Tech), Blacksburg, VA (United States). Bradley Dept. of Electrical and Computer Engineering
Publication Date:
Research Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
National Aeronautic and Space Administration (NASA); National Science Foundation (NSF); USDOE; Department of Space, Government of India
OSTI Identifier:
1402608
Report Number(s):
LA-UR-16-22089
Journal ID: ISSN 2169-9380; TRN: US1703006
Grant/Contract Number:  
AC52-06NA25396
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
Journal of Geophysical Research. Space Physics
Additional Journal Information:
Journal Volume: 122; Journal Issue: 2; Journal ID: ISSN 2169-9380
Publisher:
American Geophysical Union
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 58 GEOSCIENCES; Heliospheric and Magnetospheric Physics; IMF By; Prompt penetration electric field; Equatorial ionosphere; DP2

Citation Formats

Chakrabarty, Dipu, Hui, Debrup, Rout, Diptiranjan, Sekar, R., Bhattacharyya, Archana, Reeves, Geoffrey D., and Ruohoniemi, J. M. Role of IMF By in the prompt electric field disturbances over equatorial ionosphere during a space weather event. United States: N. p., 2017. Web. doi:10.1002/2016JA022781.
Chakrabarty, Dipu, Hui, Debrup, Rout, Diptiranjan, Sekar, R., Bhattacharyya, Archana, Reeves, Geoffrey D., & Ruohoniemi, J. M. Role of IMF By in the prompt electric field disturbances over equatorial ionosphere during a space weather event. United States. doi:10.1002/2016JA022781.
Chakrabarty, Dipu, Hui, Debrup, Rout, Diptiranjan, Sekar, R., Bhattacharyya, Archana, Reeves, Geoffrey D., and Ruohoniemi, J. M. Sat . "Role of IMF By in the prompt electric field disturbances over equatorial ionosphere during a space weather event". United States. doi:10.1002/2016JA022781. https://www.osti.gov/servlets/purl/1402608.
@article{osti_1402608,
title = {Role of IMF By in the prompt electric field disturbances over equatorial ionosphere during a space weather event},
author = {Chakrabarty, Dipu and Hui, Debrup and Rout, Diptiranjan and Sekar, R. and Bhattacharyya, Archana and Reeves, Geoffrey D. and Ruohoniemi, J. M.},
abstractNote = {On 7 January 2005 (Ap=40) prompt penetration electric field perturbations of opposite polarities were observed over Thumba and Jicamarca on a few occasions during 13:45–16:30 UT. However, the electric field was found to be eastward during 14:45–15:30 UT over both Thumba and Jicamarca contrary to the general expectation wherein opposite polarities are expected at nearly antipodal points. On closer scrutiny, three important observational features are noticed during 14:10–15:15 UT. First, during 14:10–14:45 UT, despite increasing southward interplanetary magnetic field (IMF) Bz condition, the already westward electric field over Thumba weakened (less westward) while the eastward electric field over Jicamarca intensified (more eastward). Second, the electric field not only became anomalously eastward over Thumba but also got intensified further during 14:45–15:00 UT similar to Jicamarca. Third, during 15:00–15:15 UT, despite IMF Bz remaining steadily southward, the eastward electric field continued to intensify over Thumba but weakened over Jicamarca. It is suggested that the changes in IMF By component under southward IMF Bz condition are responsible for skewing the ionospheric equipotential patterns over the dip equator in such a way that Thumba came into the same DP2 cell as that of Jicamarca leading to anomalous electric field variations. Magnetic field measurements along the Indian and Jicamarca longitude sectors and changes in high-latitude ionospheric convection patterns provide credence to this proposition. Therefore, in conclusion, the present investigation shows that the variations in IMF By are fundamentally important to understand the prompt penetration effects over low latitudes.},
doi = {10.1002/2016JA022781},
journal = {Journal of Geophysical Research. Space Physics},
number = 2,
volume = 122,
place = {United States},
year = {Sat Feb 04 00:00:00 EST 2017},
month = {Sat Feb 04 00:00:00 EST 2017}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Save / Share: