Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks

Fast forward interplanetary shocks (FFS) are characterized by positive jump in all interplanetary plasma parameters (solar wind speed, temperature and density) and interplanetary magnetic field. However the fast reverse interplanetary shocks (FRS) are characterized by negative jump in all mentioned parameters except solar wind speed. Observations show that FFS cause positive sudden impulses (SI) while FRS cause negative SI in the H-component of the geomagnetic field. In this work we investigate the SI caused by interplanetary shocks. We use the observed plasma parameters, upstream and downstream, to calculate the variation of dynamic pressure. We observe that the SI amplitude is larger for positive SI than for negative ones, as a consequence of the fact that FFS have larger dynamic pressure variations as compared to FRS.

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Main Authors: Andrioli,Vânia Fátima, Echer,Ezequiel, Savian,Jairo Francisco, Schuch,Nelson Jorge
Format: Digital revista
Language:English
Published: Sociedade Brasileira de Geofísica 2007
Online Access:http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600021
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spelling oai:scielo:S0102-261X20070006000212007-11-22Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocksAndrioli,Vânia FátimaEcher,EzequielSavian,Jairo FranciscoSchuch,Nelson Jorge Solar wind interplanetary shock waves sudden impulses magnetosphere Fast forward interplanetary shocks (FFS) are characterized by positive jump in all interplanetary plasma parameters (solar wind speed, temperature and density) and interplanetary magnetic field. However the fast reverse interplanetary shocks (FRS) are characterized by negative jump in all mentioned parameters except solar wind speed. Observations show that FFS cause positive sudden impulses (SI) while FRS cause negative SI in the H-component of the geomagnetic field. In this work we investigate the SI caused by interplanetary shocks. We use the observed plasma parameters, upstream and downstream, to calculate the variation of dynamic pressure. We observe that the SI amplitude is larger for positive SI than for negative ones, as a consequence of the fact that FFS have larger dynamic pressure variations as compared to FRS.info:eu-repo/semantics/openAccessSociedade Brasileira de GeofísicaRevista Brasileira de Geofísica v.25 suppl.2 20072007-01-01info:eu-repo/semantics/articletext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600021en10.1590/S0102-261X2007000600021
institution SCIELO
collection OJS
country Brasil
countrycode BR
component Revista
access En linea
databasecode rev-scielo-br
tag revista
region America del Sur
libraryname SciELO
language English
format Digital
author Andrioli,Vânia Fátima
Echer,Ezequiel
Savian,Jairo Francisco
Schuch,Nelson Jorge
spellingShingle Andrioli,Vânia Fátima
Echer,Ezequiel
Savian,Jairo Francisco
Schuch,Nelson Jorge
Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks
author_facet Andrioli,Vânia Fátima
Echer,Ezequiel
Savian,Jairo Francisco
Schuch,Nelson Jorge
author_sort Andrioli,Vânia Fátima
title Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks
title_short Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks
title_full Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks
title_fullStr Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks
title_full_unstemmed Positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks
title_sort positive and negative sudden impulses caused by fast forward and reverse interplanetary shocks
description Fast forward interplanetary shocks (FFS) are characterized by positive jump in all interplanetary plasma parameters (solar wind speed, temperature and density) and interplanetary magnetic field. However the fast reverse interplanetary shocks (FRS) are characterized by negative jump in all mentioned parameters except solar wind speed. Observations show that FFS cause positive sudden impulses (SI) while FRS cause negative SI in the H-component of the geomagnetic field. In this work we investigate the SI caused by interplanetary shocks. We use the observed plasma parameters, upstream and downstream, to calculate the variation of dynamic pressure. We observe that the SI amplitude is larger for positive SI than for negative ones, as a consequence of the fact that FFS have larger dynamic pressure variations as compared to FRS.
publisher Sociedade Brasileira de Geofísica
publishDate 2007
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600021
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AT savianjairofrancisco positiveandnegativesuddenimpulsescausedbyfastforwardandreverseinterplanetaryshocks
AT schuchnelsonjorge positiveandnegativesuddenimpulsescausedbyfastforwardandreverseinterplanetaryshocks
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