Published June 1, 1974 | Version v1
Journal article

ULF geomagnetic power near L = 4. III. Statistical study of power spectra in conjugate areas during December solstice

  • 1. Univ. of Nebraska, Lincoln

Description

Results are reported of statistical studies of 2-hour power spectra of nonoverlapping H component magnetic record segments. The records were obtained in January 1972 at an antarctic magnetometer station (Siple) near L=4 and at three stations (L ∼4.4, ∼4.0, ∼3.2) at approximately the same magnetic longitude in the northern conjugate area. The K index measured near the longitude of the stations was ≤5 during the interval studied. (The explicit dependence of magnetic power on geomagnetic activity is examined in part four of this series (Lanzerotti and Surkan, 1974).) It is found in the present paper that during more disturbed periods, higher power levels are accompanied by steeper spectral slopes; this finding implies a concentration of energy at the lower frequencies at these times. Relatively higher power levels are observed during the local afternoon and late evening than during other periods of the day. On the basis of power levels and spectral slopes, Siple (L ∼ 4) is more nearly conjugate to a northern station at L ∼4.4 than to a station at L ∼4 during the 1971–1972 December solstice period. This finding may arise from hemispherical differences in ionospheric conductivities and, as such, may be dependent upon season.

Additional details

Identifiers

Publishing Information

Journal Title
Journal of Geophysical Research
Journal Volume
79
Journal Issue
16
Series
J. Geophys. Res.
Journal Page Range
2403-2412
ISSN
0148-0227

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
6165401
Subject category
S58: GEOSCIENCES;
Descriptors DEI
ELECTRIC CONDUCTIVITY; ENERGY; ENERGY SPECTRA; GEOMAGNETIC FIELD; IONOSPHERE; RADIOWAVE RADIATION
Descriptors DEC
EARTH ATMOSPHERE; ELECTRICAL PROPERTIES; ELECTROMAGNETIC RADIATION; MAGNETIC FIELDS; PHYSICAL PROPERTIES; RADIATIONS; SPECTRA

Optional Information

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