Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms

Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring curr...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Zhao, Hong [verfasserIn] Zong, QiuGang [verfasserIn] Wei, Yong [verfasserIn] Wang, YongFu [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2011

Schlagwörter:	corrected index pressure correction geomagnetic storms with different intensity

Übergeordnetes Werk:	Enthalten in: Science in China - Heidelberg : Springer, 1997, 54(2011), 6 vom: 16. Apr., Seite 1445-1454
Übergeordnetes Werk:	volume:54 ; year:2011 ; number:6 ; day:16 ; month:04 ; pages:1445-1454

Links:	Volltext

DOI / URN:	10.1007/s11431-011-4319-y

Katalog-ID:	SPR019270852

Internformat


LEADER	01000caa a22002652 4500
001	SPR019270852
003	DE-627
005	20220111065405.0
007	cr uuu---uuuuu
008	201006s2011 xx \|\|\|\|\|o 00\| \|\|eng c
024	7		\|a 10.1007/s11431-011-4319-y \|2 doi
035			\|a (DE-627)SPR019270852
035			\|a (SPR)s11431-011-4319-y-e
040			\|a DE-627 \|b ger \|c DE-627 \|e rakwb
041			\|a eng
082	0	4	\|a 600 \|q ASE
082	0	4	\|a 600 \|q ASE
084			\|a 50.00 \|2 bkl
100	1		\|a Zhao, Hong \|e verfasserin \|4 aut
245	1	0	\|a Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms
264		1	\|c 2011
336			\|a Text \|b txt \|2 rdacontent
337			\|a Computermedien \|b c \|2 rdamedia
338			\|a Online-Ressource \|b cr \|2 rdacarrier
520			\|a Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min).
650		4	\|a corrected \|7 (dpeaa)DE-He213
650		4	\|a index \|7 (dpeaa)DE-He213
650		4	\|a pressure correction \|7 (dpeaa)DE-He213
650		4	\|a geomagnetic storms with different intensity \|7 (dpeaa)DE-He213
700	1		\|a Zong, QiuGang \|e verfasserin \|4 aut
700	1		\|a Wei, Yong \|e verfasserin \|4 aut
700	1		\|a Wang, YongFu \|e verfasserin \|4 aut
773	0	8	\|i Enthalten in \|t Science in China \|d Heidelberg : Springer, 1997 \|g 54(2011), 6 vom: 16. Apr., Seite 1445-1454 \|w (DE-627)385614756 \|w (DE-600)2142897-9 \|x 1862-281X \|7 nnns
773	1	8	\|g volume:54 \|g year:2011 \|g number:6 \|g day:16 \|g month:04 \|g pages:1445-1454
856	4	0	\|u https://dx.doi.org/10.1007/s11431-011-4319-y \|z lizenzpflichtig \|3 Volltext
912			\|a GBV_USEFLAG_A
912			\|a SYSFLAG_A
912			\|a GBV_SPRINGER
912			\|a GBV_ILN_20
912			\|a GBV_ILN_22
912			\|a GBV_ILN_23
912			\|a GBV_ILN_24
912			\|a GBV_ILN_31
912			\|a GBV_ILN_32
912			\|a GBV_ILN_39
912			\|a GBV_ILN_40
912			\|a GBV_ILN_60
912			\|a GBV_ILN_62
912			\|a GBV_ILN_65
912			\|a GBV_ILN_69
912			\|a GBV_ILN_70
912			\|a GBV_ILN_73
912			\|a GBV_ILN_74
912			\|a GBV_ILN_90
912			\|a GBV_ILN_95
912			\|a GBV_ILN_100
912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_120
912			\|a GBV_ILN_138
912			\|a GBV_ILN_152
912			\|a GBV_ILN_161
912			\|a GBV_ILN_171
912			\|a GBV_ILN_187
912			\|a GBV_ILN_224
912			\|a GBV_ILN_250
912			\|a GBV_ILN_281
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_702
936	b	k	\|a 50.00 \|q ASE
951			\|a AR
952			\|d 54 \|j 2011 \|e 6 \|b 16 \|c 04 \|h 1445-1454

Indexfelder

author_variant	h z hz q z qz y w yw y w yw
matchkey_str	article:1862281X:2011----::nlecoslridyaipesrogoantcsidxui
hierarchy_sort_str	2011
bklnumber	50.00
publishDate	2011
allfields	10.1007/s11431-011-4319-y doi (DE-627)SPR019270852 (SPR)s11431-011-4319-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhao, Hong verfasserin aut Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min). corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 pressure correction (dpeaa)DE-He213 geomagnetic storms with different intensity (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wei, Yong verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 6 vom: 16. Apr., Seite 1445-1454 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:6 day:16 month:04 pages:1445-1454 https://dx.doi.org/10.1007/s11431-011-4319-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 54 2011 6 16 04 1445-1454
spelling	10.1007/s11431-011-4319-y doi (DE-627)SPR019270852 (SPR)s11431-011-4319-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhao, Hong verfasserin aut Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min). corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 pressure correction (dpeaa)DE-He213 geomagnetic storms with different intensity (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wei, Yong verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 6 vom: 16. Apr., Seite 1445-1454 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:6 day:16 month:04 pages:1445-1454 https://dx.doi.org/10.1007/s11431-011-4319-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 54 2011 6 16 04 1445-1454
allfields_unstemmed	10.1007/s11431-011-4319-y doi (DE-627)SPR019270852 (SPR)s11431-011-4319-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhao, Hong verfasserin aut Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min). corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 pressure correction (dpeaa)DE-He213 geomagnetic storms with different intensity (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wei, Yong verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 6 vom: 16. Apr., Seite 1445-1454 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:6 day:16 month:04 pages:1445-1454 https://dx.doi.org/10.1007/s11431-011-4319-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 54 2011 6 16 04 1445-1454
allfieldsGer	10.1007/s11431-011-4319-y doi (DE-627)SPR019270852 (SPR)s11431-011-4319-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhao, Hong verfasserin aut Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min). corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 pressure correction (dpeaa)DE-He213 geomagnetic storms with different intensity (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wei, Yong verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 6 vom: 16. Apr., Seite 1445-1454 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:6 day:16 month:04 pages:1445-1454 https://dx.doi.org/10.1007/s11431-011-4319-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 54 2011 6 16 04 1445-1454
allfieldsSound	10.1007/s11431-011-4319-y doi (DE-627)SPR019270852 (SPR)s11431-011-4319-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhao, Hong verfasserin aut Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min). corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 pressure correction (dpeaa)DE-He213 geomagnetic storms with different intensity (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wei, Yong verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 6 vom: 16. Apr., Seite 1445-1454 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:6 day:16 month:04 pages:1445-1454 https://dx.doi.org/10.1007/s11431-011-4319-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 54 2011 6 16 04 1445-1454
language	English
source	Enthalten in Science in China 54(2011), 6 vom: 16. Apr., Seite 1445-1454 volume:54 year:2011 number:6 day:16 month:04 pages:1445-1454
sourceStr	Enthalten in Science in China 54(2011), 6 vom: 16. Apr., Seite 1445-1454 volume:54 year:2011 number:6 day:16 month:04 pages:1445-1454
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	corrected index pressure correction geomagnetic storms with different intensity
dewey-raw	600
isfreeaccess_bool	false
container_title	Science in China
authorswithroles_txt_mv	Zhao, Hong @@aut@@ Zong, QiuGang @@aut@@ Wei, Yong @@aut@@ Wang, YongFu @@aut@@
publishDateDaySort_date	2011-04-16T00:00:00Z
hierarchy_top_id	385614756
dewey-sort	3600
id	SPR019270852
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR019270852</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111065405.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201006s2011 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11431-011-4319-y</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR019270852</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11431-011-4319-y-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">50.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Zhao, Hong</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2011</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min).</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">corrected</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">index</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">pressure correction</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">geomagnetic storms with different intensity</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zong, QiuGang</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wei, Yong</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wang, YongFu</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Science in China</subfield><subfield code="d">Heidelberg : Springer, 1997</subfield><subfield code="g">54(2011), 6 vom: 16. Apr., Seite 1445-1454</subfield><subfield code="w">(DE-627)385614756</subfield><subfield code="w">(DE-600)2142897-9</subfield><subfield code="x">1862-281X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:54</subfield><subfield code="g">year:2011</subfield><subfield code="g">number:6</subfield><subfield code="g">day:16</subfield><subfield code="g">month:04</subfield><subfield code="g">pages:1445-1454</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://dx.doi.org/10.1007/s11431-011-4319-y</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_SPRINGER</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_32</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_65</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_74</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_90</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_100</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_120</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_138</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_152</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_171</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_187</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_224</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_250</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_281</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_702</subfield></datafield><datafield tag="936" ind1="b" ind2="k"><subfield code="a">50.00</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">54</subfield><subfield code="j">2011</subfield><subfield code="e">6</subfield><subfield code="b">16</subfield><subfield code="c">04</subfield><subfield code="h">1445-1454</subfield></datafield></record></collection>
author	Zhao, Hong
spellingShingle	Zhao, Hong ddc 600 bkl 50.00 misc corrected misc index misc pressure correction misc geomagnetic storms with different intensity Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms
authorStr	Zhao, Hong
ppnlink_with_tag_str_mv	@@773@@(DE-627)385614756
format	electronic Article
dewey-ones	600 - Technology
delete_txt_mv	keep
author_role	aut aut aut aut
collection	springer
remote_str	true
illustrated	Not Illustrated
issn	1862-281X
topic_title	600 ASE 50.00 bkl Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 pressure correction (dpeaa)DE-He213 geomagnetic storms with different intensity (dpeaa)DE-He213
topic	ddc 600 bkl 50.00 misc corrected misc index misc pressure correction misc geomagnetic storms with different intensity
topic_unstemmed	ddc 600 bkl 50.00 misc corrected misc index misc pressure correction misc geomagnetic storms with different intensity
topic_browse	ddc 600 bkl 50.00 misc corrected misc index misc pressure correction misc geomagnetic storms with different intensity
format_facet	Elektronische Aufsätze Aufsätze Elektronische Ressource
format_main_str_mv	Text Zeitschrift/Artikel
carriertype_str_mv	cr
hierarchy_parent_title	Science in China
hierarchy_parent_id	385614756
dewey-tens	600 - Technology
hierarchy_top_title	Science in China
isfreeaccess_txt	false
familylinks_str_mv	(DE-627)385614756 (DE-600)2142897-9
title	Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms
ctrlnum	(DE-627)SPR019270852 (SPR)s11431-011-4319-y-e
title_full	Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms
author_sort	Zhao, Hong
journal	Science in China
journalStr	Science in China
lang_code	eng
isOA_bool	false
dewey-hundreds	600 - Technology
recordtype	marc
publishDateSort	2011
contenttype_str_mv	txt
container_start_page	1445
author_browse	Zhao, Hong Zong, QiuGang Wei, Yong Wang, YongFu
container_volume	54
class	600 ASE 50.00 bkl
format_se	Elektronische Aufsätze
author-letter	Zhao, Hong
doi_str_mv	10.1007/s11431-011-4319-y
dewey-full	600
author2-role	verfasserin
title_sort	influence of solar wind dynamic pressure on geomagnetic dst index during various magnetic storms
title_auth	Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms
abstract	Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min).
abstractGer	Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min).
abstract_unstemmed	Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min).
collection_details	GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702
container_issue	6
title_short	Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms
url	https://dx.doi.org/10.1007/s11431-011-4319-y
remote_bool	true
author2	Zong, QiuGang Wei, Yong Wang, YongFu
author2Str	Zong, QiuGang Wei, Yong Wang, YongFu
ppnlink	385614756
mediatype_str_mv	c
isOA_txt	false
hochschulschrift_bool	false
doi_str	10.1007/s11431-011-4319-y
up_date	2024-07-04T00:54:31.045Z
_version_	1803607837033627648
fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR019270852</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111065405.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201006s2011 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11431-011-4319-y</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR019270852</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11431-011-4319-y-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">50.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Zhao, Hong</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2011</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The Dst index, designed as a proxy of ring current intensity, is known to be also affected by other magnetospheric current systems, e.g. magnetopause current. The pressure-corrected Dst index is obtained by removing the effects of the solar wind dynamic pressure and the quiet time ring current. However, all previous studies treated the correction coefficient as an averaged parameter for storms of different intensity. In this paper, based on the Burton’s equations and employing two independent methods, we will show a positive correlation between pressure-correction coefficient b and the intensity of the storms. We divided our storm database (872 storms in total) into three categories according to the intensity of storms. In order to improve the accuracy of calculating, we also used the higher-resolution SYM-H index data instead of Dst index to compute the corrected Dst index during different storms. Furthermore, we are able to provide corrected magnetic storm index with high-time resolution (∼ 1 min).</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">corrected</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">index</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">pressure correction</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">geomagnetic storms with different intensity</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zong, QiuGang</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wei, Yong</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wang, YongFu</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Science in China</subfield><subfield code="d">Heidelberg : Springer, 1997</subfield><subfield code="g">54(2011), 6 vom: 16. Apr., Seite 1445-1454</subfield><subfield code="w">(DE-627)385614756</subfield><subfield code="w">(DE-600)2142897-9</subfield><subfield code="x">1862-281X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:54</subfield><subfield code="g">year:2011</subfield><subfield code="g">number:6</subfield><subfield code="g">day:16</subfield><subfield code="g">month:04</subfield><subfield code="g">pages:1445-1454</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://dx.doi.org/10.1007/s11431-011-4319-y</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_SPRINGER</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_32</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_65</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_74</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_90</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_100</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_120</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_138</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_152</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_171</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_187</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_224</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_250</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_281</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_702</subfield></datafield><datafield tag="936" ind1="b" ind2="k"><subfield code="a">50.00</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">54</subfield><subfield code="j">2011</subfield><subfield code="e">6</subfield><subfield code="b">16</subfield><subfield code="c">04</subfield><subfield code="h">1445-1454</subfield></datafield></record></collection>
score	7.399596

Nicht das Richtige dabei?

Schreiben Sie uns!

Influence of solar wind dynamic pressure on geomagnetic Dst index during various magnetic storms

Nicht das Richtige dabei?

Zugang & Verfügbarkeit

Vorhandene Bände

Nicht das Richtige dabei?