Published 2009 | Version v1
Miscellaneous

GPS scintillation two low magnetic latitude stations in Brazil during the 2008-2009 prolonged solar minimum

  • 1. Universidade Federal do Rio Grande do Norte, UFRN. CCET/DGEF. Natal, RN (Brazil)
  • 2. Instituto Nacional de Pesquisas Espaciais, INPE. DAE/CEA. Sao Jose dos Campos, SP (Brazil)

Description

Complete text of publication follows. GPS scintillations are caused by irregularities in the ionospheric plasma density. At low magnetic latitudes, irregularities occur mostly just after sunset, due to an increase in the eastward electric field, the pre-reversal enhancement electric field, a phenomenon due to the ionospheric dynamo. This intense eastward electric field drives the plasma up fast and usually causes the formation of plasma density irregularities. These plasma irregularities cause ionospheric scintillations, which are fluctuations in radio signals received from artificial satellites or natural sources like stars and galaxies. Scintillations are intense during periods of maximum solar activity. Now, however, they are very weak, especially in GPS signals, since the Sun has stationed around a minimum of activity. It is believed that plasma bubbles originate at the magnetic equator and then 'propagate' through higher latitudes by moving up and diffusing along magnetic field lines. For this reason, only very low latitudes show scintillations, now. We have chosen two low latitude stations, almost aligned with the same magnetic meridian, Sao Luis (dip -4.5 deg, at 300 km) and Natal (dip -28 deg, at 300 km) both with a -20 deg declination. Scintillations were recorded at both stations at the rate of 50 samples per second per satellite, for the period of September/2008 through March/2009. To compare the scintillations at both stations the S4 index is averaged first hourly, for all satellites, and then for the whole night for all satellites. A surprising result is that it is not clear from the data that the irregularities are being produced at the lower latitude station and then moving to the higher latitude station. Some results show an increase of scintillations in Natal, which does not occur in Sao Luis. These results are discussed in terms of production of irregularities at Natal, at Sao Luis, and at other sites, eastwards, and then moving west to these stations.

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
41092752
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Non-conventional Literature
Descriptors DEI
BRAZIL; ELECTRIC FIELDS; IONOSPHERE; PLASMA DENSITY; SATELLITES; SCINTILLATIONS; SOLAR ACTIVITY
Descriptors DEC
DEVELOPING COUNTRIES; EARTH ATMOSPHERE; LATIN AMERICA; SOUTH AMERICA; STELLAR ACTIVITY

Optional Information