scholarly journals Heppa III intercomparison experiment on electron precipitation impacts, part II: Model‐measurement intercomparison of nitric oxide (NO) during a geomagnetic storm in April 2010

2021 ◽  
Author(s):  
M. Sinnhuber ◽  
H. Nesse Tyssoy ◽  
T. Asikainen ◽  
S. Bender ◽  
B. Funke ◽  
...  
Keyword(s):  
Nitric Oxide ◽  
Geomagnetic Storm ◽  
Electron Precipitation ◽  
Model Measurement

scholarly journals The effect of energetic electron precipitation on middle mesospheric night-time ozone during and after a moderate geomagnetic storm

2012 ◽  
Vol 39 (21) ◽  
pp. n/a-n/a ◽  
Author(s):  
M. Daae ◽  
P. Espy ◽  
H. Nesse Tyssøy ◽  
D. Newnham ◽  
J. Stadsnes ◽  
...  
Keyword(s):  
Geomagnetic Storm ◽  
Energetic Electron ◽  
Electron Precipitation ◽  
Night Time

scholarly journals Radiation belt electron precipitation into the atmosphere: Recovery from a geomagnetic storm

2007 ◽  
Vol 112 (A11) ◽  
pp. n/a-n/a ◽  
Author(s):  
Craig J. Rodger ◽  
Mark A. Clilverd ◽  
Neil R. Thomson ◽  
Rory J. Gamble ◽  
Annika Seppälä ◽  
...  
Keyword(s):  
Geomagnetic Storm ◽  
Radiation Belt ◽  
Electron Precipitation

scholarly journals Understanding the Behaviors of Thermospheric Nitric Oxide Cooling During the 15 May 2005 Geomagnetic Storm

2019 ◽  
Vol 124 (3) ◽  
pp. 2113-2126 ◽  
Author(s):  
Zheng Li ◽  
Delores Knipp ◽  
Wenbin Wang
Keyword(s):  
Nitric Oxide ◽  
Geomagnetic Storm

scholarly journals The driving mechanisms of particle precipitation during the moderate geomagnetic storm of 7 January 2005

2007 ◽  
Vol 25 (9) ◽  
pp. 2053-2068 ◽  
Author(s):  
N. Longden ◽  
F. Honary ◽  
A. J. Kavanagh ◽  
J. Manninen
Keyword(s):  
Solar Wind ◽  
Geomagnetic Storm ◽  
Geomagnetic Activity ◽  
Dynamic Pressure ◽  
Energetic Electron ◽  
Recovery Phase ◽  
Global Scale ◽  
Electron Precipitation ◽  
Particle Precipitation ◽  
Substorm Activity

Abstract. The arrival of an interplanetary coronal mass ejection (ICME) triggered a sudden storm commencement (SSC) at ~09:22 UT on the 7 January 2005. The ICME followed a quiet period in the solar wind and interplanetary magnetic field (IMF). We present global scale observations of energetic electron precipitation during the moderate geomagnetic storm driven by the ICME. Energetic electron precipitation is inferred from increases in cosmic noise absorption (CNA) recorded by stations in the Global Riometer Array (GLORIA). No evidence of CNA was observed during the first four hours of passage of the ICME or following the sudden commencement (SC) of the storm. This is consistent with the findings of Osepian and Kirkwood (2004) that SCs will only trigger precipitation during periods of geomagnetic activity or when the magnetic perturbation in the magnetosphere is substantial. CNA was only observed following enhanced coupling between the IMF and the magnetosphere, resulting from southward oriented IMF. Precipitation was observed due to substorm activity, as a result of the initial injection and particles drifting from the injection region. During the recovery phase of the storm, when substorm activity diminished, precipitation due to density driven increases in the solar wind dynamic pressure (Pdyn) were identified. A number of increases in Pdyn were shown to drive sudden impulses (SIs) in the geomagnetic field. While many of these SIs appear coincident with CNA, SIs without CNA were also observed. During this period, the threshold of geomagnetic activity required for SC driven precipitation was exceeded. This implies that solar wind density driven SIs occurring during storm recovery can drive a different response in particle precipitation to typical SCs.

Peculiarities of electron precipitation in morning sector of auroral zone during geomagnetic storm

1986 ◽  
Vol 30 (1) ◽  
pp. 79-86
Author(s):  
Yu. V. Gotselyuk ◽  
M. S. Kazaryan ◽  
S. N. Kuznetsov ◽  
Karel Kudela ◽  
Ivan Kimák ◽  
...  
Keyword(s):  
Geomagnetic Storm ◽  
Auroral Zone ◽  
Electron Precipitation ◽  
Morning Sector

scholarly journals Correction to “Radiation belt electron precipitation into the atmosphere: Recovery from a geomagnetic storm”

2010 ◽  
Vol 115 (A9) ◽  
pp. n/a-n/a ◽  
Author(s):  
Craig J. Rodger ◽  
Mark A. Clilverd ◽  
Neil R. Thomson ◽  
Rory J. Gamble ◽  
Annika Seppälä ◽  
...  
Keyword(s):  
Geomagnetic Storm ◽  
Radiation Belt ◽  
Electron Precipitation

scholarly journals Fluctuation of Lower Ionosphere Associated with Energetic Electron Precipitations during a Substorm

Atmosphere ◽  
2021 ◽  
Vol 12 (5) ◽  
pp. 573
Author(s):  
Tongxing Fu ◽  
Zhixu Wu ◽  
Peng Hu ◽  
Xin Zhang
Keyword(s):  
Radio Wave ◽  
Current Sheet ◽  
Geomagnetic Storm ◽  
Particle Interaction ◽  
Energetic Electron ◽  
Lower Ionosphere ◽  
Electron Precipitation ◽  
Electron Interaction ◽  
Energetic Electrons ◽  
Tail Current

In this paper, using the combined observations of the NOAA 16, LANL-01A, IMAGE satellites, VLF radio wave, and ground-based riometers, we study the fluctuation of lower ionosphere-associated precipitating energetic electrons during a geomagnetic storm on 8 November 2004. Associated with the substorm dispersion injection observed by the LANL-01A satellite, the riometers observed obvious enhancements of ionospheric absorption within the electron isotropic zone, which they attributed to the tail current sheet scattering (TCS) mechanism. Through observations of the NOAA 16 satellite, we found a sharp enhancement of the precipitating electron flux within the anisotropic zone, which entailed an obvious separation of energetic electron precipitation at high latitudes. This energetic electron precipitation within the anisotropic zone leads to the significant enhancement of electron density in the D region, thus resulting in the variations of VLF radio wave amplitudes, which propagate in the middle latitudes. Since the projection of the electron precipitation region within the anisotropic zone is at the inner edge of the plasmapause observed by the IMAGE EUV, the precipitation of energetic electrons should be attributed to the ELF hiss-ring current electron interaction. As a result, the energetic electron precipitations due to the tail current sheet scattering mechanism and wave-particle interaction in the inner magnetosphere were both observed and analyzed as they were associated with a substorm during a geomagnetic storm.

scholarly journals Direct observations of nitric oxide produced by energetic electron precipitation into the Antarctic middle atmosphere

2011 ◽  
Vol 38 (20) ◽  
pp. n/a-n/a ◽  
Author(s):  
David A. Newnham ◽  
Patrick J. Espy ◽  
Mark A. Clilverd ◽  
Craig J. Rodger ◽  
Annika Seppälä ◽  
...  
Keyword(s):  
Nitric Oxide ◽  
Middle Atmosphere ◽  
Energetic Electron ◽  
Electron Precipitation ◽  
Direct Observations ◽  
The Antarctic
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