Published 2009 | Version v1
Miscellaneous

Halos. A solution to the sprite polarity paradox

  • 1. Massachusetts Institute of Technology, Cambridge, MA (United States). Parsons Laboratory
  • 2. Geodetic and Geophysical Research Institute, HAS, Sopron (Hungary)
  • 3. National Central University, National Cheng Kung University, Tainan, Taiwan (China). Institute of Space Science
  • 4. National Cheng Kung University, Tainan, Taiwan (China). Department of Physics
  • 5. University of Alabama, Huntsville, AL (United States)
  • 6. National Cheng Kung University, Tainan, Taiwan (China). Institute of Space, Astrophysical and Plasma Sciences
  • 7. Earth Dynamic System Research Center, National Cheng Kung University, Tainan, Taiwan (China)
  • 8. FMA Research, Inc., Fort Collins, CO (United States)
  • 9. National Institute for Space Research, Sao Jose dos Campos (Brazil)

Description

Complete text of publication follows. C.T.R. Wilson's explanation for sprite initiation in the mesosphere by lightning in the troposphere is independent of the polarity of the parent lightning. Yet in thousands of published ground-based observations of sprites, only three have been clearly associated with ground flashes with negative polarity. This finding is however inconsistent with ELF measurements of charge moments, showing that typically 10% of supercritical values are negative in polarity. ISUAL satellite measurements in the Earth's limb have exposed a population of halos that is a substantially larger fraction of total TLEs (sprites+halos) than in the earlier ground-based measurements. ELF measurements from Nagycenk, Hungary for more than one hundreds ISUAL-identified halos show a predominant negative polarity in the parent lightning with a range of charge moments from 300-1200 C-km. Halo brightness measured by ISUAL is positively correlated with the vertical charge moment, consistent with theoretical predictions based on impact excitation of nitrogen for halo production. The polarity asymmetry in TLE production by positive and negative ground flashes appears to resolve the original sprite polarity paradox. The physical reasons for the differences in positive and negative flashes deserve further clarification.

Part of:
International Association of Geomagnetism and Aeronomy IAGA 11. Scientific Assembly

Additional details

Identifiers

Publishing Information

Publisher
Geodetic and Geophysical Research Institute of the Hungarian Academy of Sciences
Imprint Place
Sopron (Hungary)
Imprint Title
International Association of Geomagnetism and Aeronomy IAGA 11. Scientific Assembly
Imprint Pagination
[1212 p.]
Journal Page Range
[1 p.]
Report number
INIS-HU--010

Conference

Title
International Association of Geomagnetism and Aeronomy IAGA 11. Scientific Assembly
Dates
23-30 Aug 2009
Place
Sopron (Hungary)

INIS

Country of Publication
Hungary
Country of Input or Organization
Hungary
INIS RN
41084196
Subject category
S58: GEOSCIENCES;
Resource subtype / Literary indicator
Conference, Non-conventional Literature
Descriptors DEI
HUNGARY; LIGHTNING; LIMBS; NITROGEN; SATELLITES
Descriptors DEC
BODY; DEVELOPING COUNTRIES; EASTERN EUROPE; ELECTRIC DISCHARGES; ELEMENTS; EUROPE; NONMETALS

Optional Information