Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23
Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Joshi, Navin Chandra [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2009 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© Springer Science+Business Media B.V. 2009 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Solar physics - Springer Netherlands, 1967, 260(2009), 2 vom: 02. Okt., Seite 451-463 |
|---|---|
| Übergeordnetes Werk: |
volume:260 ; year:2009 ; number:2 ; day:02 ; month:10 ; pages:451-463 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11207-009-9446-2 |
|---|
| Katalog-ID: |
OLC2033606481 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2033606481 | ||
| 003 | DE-627 | ||
| 005 | 20230504045832.0 | ||
| 007 | tu | ||
| 008 | 200819s2009 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/s11207-009-9446-2 |2 doi | |
| 035 | |a (DE-627)OLC2033606481 | ||
| 035 | |a (DE-He213)s11207-009-9446-2-p | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 530 |q VZ |
| 084 | |a 16,12 |2 ssgn | ||
| 100 | 1 | |a Joshi, Navin Chandra |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 |
| 264 | 1 | |c 2009 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
| 338 | |a Band |b nc |2 rdacarrier | ||
| 500 | |a © Springer Science+Business Media B.V. 2009 | ||
| 520 | |a Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. | ||
| 650 | 4 | |a Sun: activity | |
| 650 | 4 | |a Sun: prominences | |
| 650 | 4 | |a Sun: North – South and East – West asymmetry | |
| 700 | 1 | |a Bankoti, Neeraj Singh |4 aut | |
| 700 | 1 | |a Pande, Seema |4 aut | |
| 700 | 1 | |a Pande, Bimal |4 aut | |
| 700 | 1 | |a Pandey, Kavita |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Solar physics |d Springer Netherlands, 1967 |g 260(2009), 2 vom: 02. Okt., Seite 451-463 |w (DE-627)129856010 |w (DE-600)281593-X |w (DE-576)015160033 |x 0038-0938 |7 nnns |
| 773 | 1 | 8 | |g volume:260 |g year:2009 |g number:2 |g day:02 |g month:10 |g pages:451-463 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/s11207-009-9446-2 |z lizenzpflichtig |3 Volltext |
| 912 | |a GBV_USEFLAG_A | ||
| 912 | |a SYSFLAG_A | ||
| 912 | |a GBV_OLC | ||
| 912 | |a SSG-OLC-PHY | ||
| 912 | |a SSG-OLC-AST | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_40 | ||
| 912 | |a GBV_ILN_47 | ||
| 912 | |a GBV_ILN_70 | ||
| 951 | |a AR | ||
| 952 | |d 260 |j 2009 |e 2 |b 02 |c 10 |h 451-463 | ||
| author_variant |
n c j nc ncj n s b ns nsb s p sp b p bp k p kp |
|---|---|
| matchkey_str |
article:00380938:2009----::tdodsrbtoadsmeroslrciermnne |
| hierarchy_sort_str |
2009 |
| publishDate |
2009 |
| allfields |
10.1007/s11207-009-9446-2 doi (DE-627)OLC2033606481 (DE-He213)s11207-009-9446-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Joshi, Navin Chandra verfasserin aut Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. Sun: activity Sun: prominences Sun: North – South and East – West asymmetry Bankoti, Neeraj Singh aut Pande, Seema aut Pande, Bimal aut Pandey, Kavita aut Enthalten in Solar physics Springer Netherlands, 1967 260(2009), 2 vom: 02. Okt., Seite 451-463 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:260 year:2009 number:2 day:02 month:10 pages:451-463 https://doi.org/10.1007/s11207-009-9446-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 260 2009 2 02 10 451-463 |
| spelling |
10.1007/s11207-009-9446-2 doi (DE-627)OLC2033606481 (DE-He213)s11207-009-9446-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Joshi, Navin Chandra verfasserin aut Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. Sun: activity Sun: prominences Sun: North – South and East – West asymmetry Bankoti, Neeraj Singh aut Pande, Seema aut Pande, Bimal aut Pandey, Kavita aut Enthalten in Solar physics Springer Netherlands, 1967 260(2009), 2 vom: 02. Okt., Seite 451-463 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:260 year:2009 number:2 day:02 month:10 pages:451-463 https://doi.org/10.1007/s11207-009-9446-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 260 2009 2 02 10 451-463 |
| allfields_unstemmed |
10.1007/s11207-009-9446-2 doi (DE-627)OLC2033606481 (DE-He213)s11207-009-9446-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Joshi, Navin Chandra verfasserin aut Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. Sun: activity Sun: prominences Sun: North – South and East – West asymmetry Bankoti, Neeraj Singh aut Pande, Seema aut Pande, Bimal aut Pandey, Kavita aut Enthalten in Solar physics Springer Netherlands, 1967 260(2009), 2 vom: 02. Okt., Seite 451-463 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:260 year:2009 number:2 day:02 month:10 pages:451-463 https://doi.org/10.1007/s11207-009-9446-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 260 2009 2 02 10 451-463 |
| allfieldsGer |
10.1007/s11207-009-9446-2 doi (DE-627)OLC2033606481 (DE-He213)s11207-009-9446-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Joshi, Navin Chandra verfasserin aut Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. Sun: activity Sun: prominences Sun: North – South and East – West asymmetry Bankoti, Neeraj Singh aut Pande, Seema aut Pande, Bimal aut Pandey, Kavita aut Enthalten in Solar physics Springer Netherlands, 1967 260(2009), 2 vom: 02. Okt., Seite 451-463 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:260 year:2009 number:2 day:02 month:10 pages:451-463 https://doi.org/10.1007/s11207-009-9446-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 260 2009 2 02 10 451-463 |
| allfieldsSound |
10.1007/s11207-009-9446-2 doi (DE-627)OLC2033606481 (DE-He213)s11207-009-9446-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Joshi, Navin Chandra verfasserin aut Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. Sun: activity Sun: prominences Sun: North – South and East – West asymmetry Bankoti, Neeraj Singh aut Pande, Seema aut Pande, Bimal aut Pandey, Kavita aut Enthalten in Solar physics Springer Netherlands, 1967 260(2009), 2 vom: 02. Okt., Seite 451-463 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:260 year:2009 number:2 day:02 month:10 pages:451-463 https://doi.org/10.1007/s11207-009-9446-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 260 2009 2 02 10 451-463 |
| language |
English |
| source |
Enthalten in Solar physics 260(2009), 2 vom: 02. Okt., Seite 451-463 volume:260 year:2009 number:2 day:02 month:10 pages:451-463 |
| sourceStr |
Enthalten in Solar physics 260(2009), 2 vom: 02. Okt., Seite 451-463 volume:260 year:2009 number:2 day:02 month:10 pages:451-463 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Sun: activity Sun: prominences Sun: North – South and East – West asymmetry |
| dewey-raw |
530 |
| isfreeaccess_bool |
false |
| container_title |
Solar physics |
| authorswithroles_txt_mv |
Joshi, Navin Chandra @@aut@@ Bankoti, Neeraj Singh @@aut@@ Pande, Seema @@aut@@ Pande, Bimal @@aut@@ Pandey, Kavita @@aut@@ |
| publishDateDaySort_date |
2009-10-02T00:00:00Z |
| hierarchy_top_id |
129856010 |
| dewey-sort |
3530 |
| id |
OLC2033606481 |
| 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">OLC2033606481</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045832.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2009 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11207-009-9446-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033606481</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11207-009-9446-2-p</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">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Joshi, Navin Chandra</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2009</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">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science+Business Media B.V. 2009</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Sun: activity</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Sun: prominences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Sun: North – South and East – West asymmetry</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bankoti, Neeraj Singh</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pande, Seema</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pande, Bimal</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pandey, Kavita</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">Springer Netherlands, 1967</subfield><subfield code="g">260(2009), 2 vom: 02. Okt., Seite 451-463</subfield><subfield code="w">(DE-627)129856010</subfield><subfield code="w">(DE-600)281593-X</subfield><subfield code="w">(DE-576)015160033</subfield><subfield code="x">0038-0938</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:260</subfield><subfield code="g">year:2009</subfield><subfield code="g">number:2</subfield><subfield code="g">day:02</subfield><subfield code="g">month:10</subfield><subfield code="g">pages:451-463</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s11207-009-9446-2</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_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</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_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">260</subfield><subfield code="j">2009</subfield><subfield code="e">2</subfield><subfield code="b">02</subfield><subfield code="c">10</subfield><subfield code="h">451-463</subfield></datafield></record></collection>
|
| author |
Joshi, Navin Chandra |
| spellingShingle |
Joshi, Navin Chandra ddc 530 ssgn 16,12 misc Sun: activity misc Sun: prominences misc Sun: North – South and East – West asymmetry Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 |
| authorStr |
Joshi, Navin Chandra |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)129856010 |
| format |
Article |
| dewey-ones |
530 - Physics |
| delete_txt_mv |
keep |
| author_role |
aut aut aut aut aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0038-0938 |
| topic_title |
530 VZ 16,12 ssgn Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 Sun: activity Sun: prominences Sun: North – South and East – West asymmetry |
| topic |
ddc 530 ssgn 16,12 misc Sun: activity misc Sun: prominences misc Sun: North – South and East – West asymmetry |
| topic_unstemmed |
ddc 530 ssgn 16,12 misc Sun: activity misc Sun: prominences misc Sun: North – South and East – West asymmetry |
| topic_browse |
ddc 530 ssgn 16,12 misc Sun: activity misc Sun: prominences misc Sun: North – South and East – West asymmetry |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| hierarchy_parent_title |
Solar physics |
| hierarchy_parent_id |
129856010 |
| dewey-tens |
530 - Physics |
| hierarchy_top_title |
Solar physics |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)129856010 (DE-600)281593-X (DE-576)015160033 |
| title |
Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 |
| ctrlnum |
(DE-627)OLC2033606481 (DE-He213)s11207-009-9446-2-p |
| title_full |
Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 |
| author_sort |
Joshi, Navin Chandra |
| journal |
Solar physics |
| journalStr |
Solar physics |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science |
| recordtype |
marc |
| publishDateSort |
2009 |
| contenttype_str_mv |
txt |
| container_start_page |
451 |
| author_browse |
Joshi, Navin Chandra Bankoti, Neeraj Singh Pande, Seema Pande, Bimal Pandey, Kavita |
| container_volume |
260 |
| class |
530 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Joshi, Navin Chandra |
| doi_str_mv |
10.1007/s11207-009-9446-2 |
| dewey-full |
530 |
| title_sort |
study of distribution and asymmetry of solar active prominences during solar cycle 23 |
| title_auth |
Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 |
| abstract |
Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. © Springer Science+Business Media B.V. 2009 |
| abstractGer |
Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. © Springer Science+Business Media B.V. 2009 |
| abstract_unstemmed |
Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry. © Springer Science+Business Media B.V. 2009 |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 |
| container_issue |
2 |
| title_short |
Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23 |
| url |
https://doi.org/10.1007/s11207-009-9446-2 |
| remote_bool |
false |
| author2 |
Bankoti, Neeraj Singh Pande, Seema Pande, Bimal Pandey, Kavita |
| author2Str |
Bankoti, Neeraj Singh Pande, Seema Pande, Bimal Pandey, Kavita |
| ppnlink |
129856010 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/s11207-009-9446-2 |
| up_date |
2024-07-03T17:40:24.203Z |
| _version_ |
1803580524939182080 |
| 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">OLC2033606481</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045832.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2009 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11207-009-9446-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033606481</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11207-009-9446-2-p</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">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Joshi, Navin Chandra</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Study of Distribution and Asymmetry of Solar Active Prominences during Solar Cycle 23</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2009</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">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science+Business Media B.V. 2009</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract In this article we present the results of a study of the spatial distribution and asymmetry of solar active prominences (SAP) for the period 1996 through 2007 (solar cycle 23). For more meaningful statistical analysis we analyzed the distribution and asymmetry of SAP in two subdivisions viz. Group1 (ADF, APR, DSF, CRN, CAP) and Group2 (AFS, ASR, BSD, BSL, DSD, SPY, LPS). The North – South (N – S) latitudinal distribution shows that the SAP events are most prolific in the 21° to 30° slice in the Northern and Southern Hemispheres; the East – West (E – W) longitudinal distribution study shows that the SAP events are most prolific (best observable) in the 81° to 90° slice in the Eastern and Western Hemispheres. It was found that the SAP activity during this cycle is low compared to previous solar cycles. The present study indicates that during the rising phase of the cycle the number of SAP events are roughly equal in the Northern and Southern Hemispheres. However, activity in the Southern Hemisphere has been dominant since 1999. Our statistical study shows that the N – S asymmetry is more significant then the E – W asymmetry.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Sun: activity</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Sun: prominences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Sun: North – South and East – West asymmetry</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bankoti, Neeraj Singh</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pande, Seema</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pande, Bimal</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pandey, Kavita</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">Springer Netherlands, 1967</subfield><subfield code="g">260(2009), 2 vom: 02. Okt., Seite 451-463</subfield><subfield code="w">(DE-627)129856010</subfield><subfield code="w">(DE-600)281593-X</subfield><subfield code="w">(DE-576)015160033</subfield><subfield code="x">0038-0938</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:260</subfield><subfield code="g">year:2009</subfield><subfield code="g">number:2</subfield><subfield code="g">day:02</subfield><subfield code="g">month:10</subfield><subfield code="g">pages:451-463</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s11207-009-9446-2</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_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</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_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">260</subfield><subfield code="j">2009</subfield><subfield code="e">2</subfield><subfield code="b">02</subfield><subfield code="c">10</subfield><subfield code="h">451-463</subfield></datafield></record></collection>
|
| score |
7.3988447 |