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Gonzalez, W. D., Echer, E., Tsurutani, B. T. (2008) Reply to comment by C. Cid, E. Saiz, and Y. Cerrato on “Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23”. Geophysical Research Letters, 35 (21) doi:10.1029/2008gl035164

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Reference TypeJournal (article/letter/editorial)
TitleReply to comment by C. Cid, E. Saiz, and Y. Cerrato on “Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23”
JournalGeophysical Research Letters
AuthorsGonzalez, W. D.Author
Echer, E.Author
Tsurutani, B. T.Author
Year2008 (November 15)Volume35
Issue21
PublisherAmerican Geophysical Union (AGU)
DOIdoi:10.1029/2008gl035164Search in ResearchGate
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Mindat Ref. ID831330Long-form Identifiermindat:1:5:831330:4
GUID0
Full ReferenceGonzalez, W. D., Echer, E., Tsurutani, B. T. (2008) Reply to comment by C. Cid, E. Saiz, and Y. Cerrato on “Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23”. Geophysical Research Letters, 35 (21) doi:10.1029/2008gl035164
Plain TextGonzalez, W. D., Echer, E., Tsurutani, B. T. (2008) Reply to comment by C. Cid, E. Saiz, and Y. Cerrato on “Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23”. Geophysical Research Letters, 35 (21) doi:10.1029/2008gl035164
In(2008, November) Geophysical Research Letters Vol. 35 (21) American Geophysical Union (AGU)

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Cid, C., Saiz, E., Cerrato, Y. (2008) Comment on “Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23” by E. Echer et al. Geophysical Research Letters, 35 (21) doi:10.1029/2008gl034731
Echer, E., Gonzalez, W. D., Tsurutani, B. T. (2008) Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23. Geophysical Research Letters, 35 (6) doi:10.1029/2007gl031755
Gonzalez, W. D., Echer, E., Clua de Gonzalez, A. L., Tsurutani, B. T. (2008) Reply to comment by Y. I. Yermolaev and M. Y. Yermolaev on “Interplanetary origin of intense geomagnetic storms (Dst< −100 nT) during solar cycle 23”. Geophysical Research Letters, 35 (1) doi:10.1029/2007gl031856
Echer, E., Gonzalez, W. D., Tsurutani, B. T., Gonzalez, A. L. C. (2008) Interplanetary conditions causing intense geomagnetic storms (Dst ≤ −100 nT) during solar cycle 23 (1996-2006). Journal of Geophysical Research: Space Physics, 113. doi:10.1029/2007ja012744
Gonzalez, W. D., Echer, E., Clua-Gonzalez, A. L., Tsurutani, B. T. (2007) Interplanetary origin of intense geomagnetic storms (Dst< −100 nT) during solar cycle 23. Geophysical Research Letters, 34 (6) doi:10.1029/2006gl028879
Yermolaev, Y. I., Yermolaev, M. Y. (2008) Comment on “Interplanetary origin of intense geomagnetic storms (Dst< −100 nT) during solar cycle 23” by W. D. Gonzalez et al. Geophysical Research Letters, 35 (1) doi:10.1029/2007gl030281
Tsurutani, Bruce T., Gonzalez, Walter D. (1990) Reply [to “Comment on ‘Solar sources of interplanetary southward Bzevents responsible for major magnetic storms (1978–1979)’ by F. Tang, B. T. Tsurutani, W. D. Gonzalez, S. I. Akasofu, and E. J. Smith”]. Journal of Geophysical Research, 95. 12305 doi:10.1029/ja095ia08p12305
Aguado, J., Cid, C., Saiz, E., Cerrato, Y. (2010) Hyperbolic decay of the Dst Index during the recovery phase of intense geomagnetic storms. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2009ja014658
Echer, E., Tsurutani, B. T., Gonzalez, W. D. (2013) Interplanetary origins of moderate (−100 nT Journal of Geophysical Research: Space Physics, 118 (1). 385-392 doi:10.1029/2012ja018086
Gonzalez, W. D., Echer, E. (2005) A study on the peak Dst and peak negative Bz relationship during intense geomagnetic storms. Geophysical Research Letters, 32 (18) doi:10.1029/2005gl023486
Tsurutani, Bruce, Gonzalez, Walter D., Tang, Frances M. (1996) Reply [to “Comment on ‘Interplanetary origin of geomagnetic activity in the declining phase of the solar cycle’ by B. T. Tsurutani et al.”]. Journal of Geophysical Research: Space Physics, 101. 27631-27633 doi:10.1029/96ja02499
 
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