Atmospheric electric field anomalies associated with solar flare/coronal mass ejection events and solar energetic charged particle

Abstract. We discuss the fair weather atmospheric electric field signatures of three major solar energetic charged particle events which occurred in on 15 April 2001, 18 April and 4 November, and their causative solar flares/coronal mass ejections (SF/CMEs). Only the 15 April 2001 shows clear evidence for Ez variation associated to SF/CME events and the other two events may support this hypothesis as well although for them the meteorological data were not available. All three events seem to be associated with relativistic solar protons (i.e. protons with energies >450 MeV) of the Ground Level Event (GLE) type. The study presents data on variations of the vertical component of the atmospheric electric field (Ez) measured at the auroral station Apatity (geomagnetic latitude: 63.8°, the polar cap station Vostok (geomagnetic latitude: −89.3°) and the middle latitude stations Voyeikovo (geomagnetic latitude: 56.1°) and Nagycenk (geomagnetic latitude: 47.2°). A significant disturbance in the atmospheric electric field is sometimes observed close to the time of the causative solar flare; the beginning of the electric field perturbation at Apatity is detected one or two hours before the flare onset and the GLE onset. Atmospheric electric field records at Vostok and Voyeikovo show a similar disturbance at the same time for the 15 April 2001 event. Some mechanisms responsible for the electric field perturbations are considered.

[1]  O. Shumilov,et al.  Cosmic ray-induced stratospheric aerosols: A possible connection to polar ozone depletions , 2005 .

[2]  V. Romano,et al.  Polar cap absorption events of November 2001 at Terra Nova Bay, Antarctica , 2004 .

[3]  R. G. Harrison,et al.  Long-term changes in atmospheric electrical parameters observed at Nagycenk (Hungary) and the UK observatories at Eskdalemuir and Kew , 2003 .

[4]  N. Raouafi,et al.  Far-Ultraviolet Spectra of Fast Coronal Mass Ejections Associated with X-Class Flares , 2003, astro-ph/0308058.

[5]  C. Sastry,et al.  Metric Radio Observations of the Evolution of a “Halo” Coronal Mass Ejection Close to the Sun , 2003 .

[6]  R. Mewaldt,et al.  Two components in major solar particle events , 2003 .

[7]  N. Gopalswamy,et al.  Large solar energetic particle events of cycle 23: A global view , 2003 .

[8]  E. Cliver,et al.  Low Coronal Signatures of Large Solar Energetic Particle Events , 2003 .

[9]  S. Kahler,et al.  Solar Energetic Particle Production by Coronal Mass Ejection-driven Shocks in Solar Fast-Wind Regions , 2003 .

[10]  D. Haggerty,et al.  The Acceleration and Release of Near-relativistic Electrons by Coronal Mass Ejections , 2002 .

[11]  Edmond C. Roelof,et al.  Impulsive Near-relativistic Solar Electron Events: Delayed Injection with Respect to Solar Electromagnetic Emission , 2002 .

[12]  C. D'Andrea,et al.  Ground level muons in coincidence with the solar flare of 15 April 2001 , 2002, astro-ph/0211490.

[13]  R. Ramesh,et al.  Decameter Wavelength Observations of an Absorption Burst from the Sun and Its Association with an X2.0/3B Flare and the Onset of a “Halo” Coronal Mass Ejection , 2001 .

[14]  Angelos Vourlidas,et al.  The Coronal Mass Ejection of 1998 April 20: Direct Imaging at Radio Wavelengths , 2001 .

[15]  A. Vourlidas,et al.  Nonthermal Radio Signatures of Coronal Disturbances with and without Coronal Mass Ejections , 1999 .

[16]  A. Zadorozhny,et al.  Effects of geomagnetic activity on the mesospheric electric fields , 1998 .

[17]  F. Märcz Short-term changes in atmospheric electricity associated with Forbush decreases , 1997 .

[18]  O. Shumilov,et al.  Enhancement of stratospheric aerosols after solar proton event , 1996 .

[19]  A. Zadorozhny,et al.  Middle atmosphere response to the solar proton events of October 1989 using the results of rocket measurements , 1994 .

[20]  D. Baker,et al.  Energy deposition and middle atmosphere electrodynamic response to a highly relativistic electron precipitation event , 1994 .

[21]  A. Yaroshenko,et al.  Space‐time structure and reasons of global, regional, and local variations of atmospheric electricity , 1994 .

[22]  M. Hudson,et al.  Simulation of the prompt energization and transport of radiation belt particles during the March 24, 1991 SSC , 1993 .

[23]  J. Gosling The solar flare myth , 1993 .

[24]  O. Shumilov,et al.  Quasi-drift effects of high-energy solar cosmic rays in the magnetosphere , 1993 .

[25]  W. Kolasinski,et al.  Injection of electrons and protons with energies of tens of MeV into L < 3 on 24 March 1991. (Reannouncement with new availability information) , 1992 .

[26]  A. Aikin,et al.  A Van de Graaf source mechanism for middle atmospheric vertical electric fields , 1990 .

[27]  R. Holzworth,et al.  Solar flare perturbations in stratospheric current systems , 1987 .

[28]  R. A. Goldberg Middle atmospheric electrodynamics : status and future , 1984 .

[29]  J. E. Evans,et al.  The effects of energetic particle precipitation on the atmospheric electric circuit , 1983 .

[30]  D. Hofmann,et al.  Condensation nuclei events at 30 km and possible influences of solar cosmic rays , 1983, Nature.

[31]  F. Arnold,et al.  Ion nucleation—a potential source for stratospheric aerosols , 1982, Nature.

[32]  L. Hale,et al.  An auroral effect on the fair weather electric field , 1979, Nature.

[33]  F. Mozer,et al.  Direct evidence of solar flare modification of stratospheric electric fields , 1979 .

[34]  R. H. Olson,et al.  Solar plages and the vorticity of the Earth's atmosphere , 1978, Nature.

[35]  Ralph Markson,et al.  Solar modulation of atmospheric electrification and possible implications for the Sun–weather relationship , 1978, Nature.

[36]  F. Märcz Links between atmospheric electricity and ionospheric absorption due to extraterrestrial influences , 1976 .

[37]  R. Markson Considerations regarding solar and lunar modulation of geophysical parameters, atmospheric electricity and thunderstorms , 1971 .

[38]  R. Reiter Solar flares and their impact on potential gradient and air-earth current characteristics at high mountain stations , 1969 .

[39]  W. E. Cobb Evidence of a Solar Influence on the Atmospheric Electric Elements at Mauna Loa Observatory , 1967 .

[40]  M. Born Space–Time Structure , 1951, Nature.

[41]  M. J. Rycrofta,et al.  The global atmospheric electric circuit , solar activity and climate change , 2000 .

[42]  A. Mitra Polar Cap Absorption Events , 1974 .

[43]  E. B. Mayfield,et al.  Variations in solar emission at 3.3 mm wavelength and their relation to flares , 1970 .