Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly
Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the rec...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Bazilevskaya, G. A. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1994 |
|---|
| Anmerkung: |
© Società Italiana di Fisica 1994 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Il Nuovo Cimento C - Kluwer Academic Publishers, 1978, 17(1994), 2 vom: März, Seite 223-235 |
|---|---|
| Übergeordnetes Werk: |
volume:17 ; year:1994 ; number:2 ; month:03 ; pages:223-235 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF02508588 |
|---|
| Katalog-ID: |
OLC2055372955 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2055372955 | ||
| 003 | DE-627 | ||
| 005 | 20230401104628.0 | ||
| 007 | tu | ||
| 008 | 200819s1994 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/BF02508588 |2 doi | |
| 035 | |a (DE-627)OLC2055372955 | ||
| 035 | |a (DE-He213)BF02508588-p | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 530 |q VZ |
| 084 | |a 16,13 |2 ssgn | ||
| 100 | 1 | |a Bazilevskaya, G. A. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| 264 | 1 | |c 1994 | |
| 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 © Società Italiana di Fisica 1994 | ||
| 520 | |a Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. | ||
| 700 | 1 | |a Bui-Van, N. A. |4 aut | |
| 700 | 1 | |a Kvashnin, A. N. |4 aut | |
| 700 | 1 | |a Martin, I. M. |4 aut | |
| 700 | 1 | |a Mizin, S. V. |4 aut | |
| 700 | 1 | |a Podgorny, A. I. |4 aut | |
| 700 | 1 | |a Stozhkov, Yu. I. |4 aut | |
| 700 | 1 | |a Turtelli, A. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Il Nuovo Cimento C |d Kluwer Academic Publishers, 1978 |g 17(1994), 2 vom: März, Seite 223-235 |w (DE-627)129367362 |w (DE-600)161886-6 |w (DE-576)014741970 |x 1124-1896 |7 nnns |
| 773 | 1 | 8 | |g volume:17 |g year:1994 |g number:2 |g month:03 |g pages:223-235 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/BF02508588 |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-GEO | ||
| 912 | |a SSG-OLC-AST | ||
| 912 | |a SSG-OPC-GGO | ||
| 912 | |a SSG-OPC-GEO | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_11 | ||
| 912 | |a GBV_ILN_20 | ||
| 912 | |a GBV_ILN_22 | ||
| 912 | |a GBV_ILN_40 | ||
| 912 | |a GBV_ILN_70 | ||
| 912 | |a GBV_ILN_130 | ||
| 912 | |a GBV_ILN_2012 | ||
| 912 | |a GBV_ILN_4046 | ||
| 912 | |a GBV_ILN_4103 | ||
| 912 | |a GBV_ILN_4155 | ||
| 951 | |a AR | ||
| 952 | |d 17 |j 1994 |e 2 |c 03 |h 223-235 | ||
| author_variant |
g a b ga gab n a b v nab nabv a n k an ank i m m im imm s v m sv svm a i p ai aip y i s yi yis a t at |
|---|---|
| matchkey_str |
article:11241896:1994----::ielcutosfhreadetacsiryopnnfueamaueiteein |
| hierarchy_sort_str |
1994 |
| publishDate |
1994 |
| allfields |
10.1007/BF02508588 doi (DE-627)OLC2055372955 (DE-He213)BF02508588-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly 1994 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1994 Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. Bui-Van, N. A. aut Kvashnin, A. N. aut Martin, I. M. aut Mizin, S. V. aut Podgorny, A. I. aut Stozhkov, Yu. I. aut Turtelli, A. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 17(1994), 2 vom: März, Seite 223-235 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:17 year:1994 number:2 month:03 pages:223-235 https://doi.org/10.1007/BF02508588 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 AR 17 1994 2 03 223-235 |
| spelling |
10.1007/BF02508588 doi (DE-627)OLC2055372955 (DE-He213)BF02508588-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly 1994 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1994 Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. Bui-Van, N. A. aut Kvashnin, A. N. aut Martin, I. M. aut Mizin, S. V. aut Podgorny, A. I. aut Stozhkov, Yu. I. aut Turtelli, A. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 17(1994), 2 vom: März, Seite 223-235 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:17 year:1994 number:2 month:03 pages:223-235 https://doi.org/10.1007/BF02508588 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 AR 17 1994 2 03 223-235 |
| allfields_unstemmed |
10.1007/BF02508588 doi (DE-627)OLC2055372955 (DE-He213)BF02508588-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly 1994 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1994 Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. Bui-Van, N. A. aut Kvashnin, A. N. aut Martin, I. M. aut Mizin, S. V. aut Podgorny, A. I. aut Stozhkov, Yu. I. aut Turtelli, A. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 17(1994), 2 vom: März, Seite 223-235 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:17 year:1994 number:2 month:03 pages:223-235 https://doi.org/10.1007/BF02508588 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 AR 17 1994 2 03 223-235 |
| allfieldsGer |
10.1007/BF02508588 doi (DE-627)OLC2055372955 (DE-He213)BF02508588-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly 1994 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1994 Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. Bui-Van, N. A. aut Kvashnin, A. N. aut Martin, I. M. aut Mizin, S. V. aut Podgorny, A. I. aut Stozhkov, Yu. I. aut Turtelli, A. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 17(1994), 2 vom: März, Seite 223-235 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:17 year:1994 number:2 month:03 pages:223-235 https://doi.org/10.1007/BF02508588 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 AR 17 1994 2 03 223-235 |
| allfieldsSound |
10.1007/BF02508588 doi (DE-627)OLC2055372955 (DE-He213)BF02508588-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly 1994 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1994 Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. Bui-Van, N. A. aut Kvashnin, A. N. aut Martin, I. M. aut Mizin, S. V. aut Podgorny, A. I. aut Stozhkov, Yu. I. aut Turtelli, A. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 17(1994), 2 vom: März, Seite 223-235 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:17 year:1994 number:2 month:03 pages:223-235 https://doi.org/10.1007/BF02508588 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 AR 17 1994 2 03 223-235 |
| language |
English |
| source |
Enthalten in Il Nuovo Cimento C 17(1994), 2 vom: März, Seite 223-235 volume:17 year:1994 number:2 month:03 pages:223-235 |
| sourceStr |
Enthalten in Il Nuovo Cimento C 17(1994), 2 vom: März, Seite 223-235 volume:17 year:1994 number:2 month:03 pages:223-235 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| dewey-raw |
530 |
| isfreeaccess_bool |
false |
| container_title |
Il Nuovo Cimento C |
| authorswithroles_txt_mv |
Bazilevskaya, G. A. @@aut@@ Bui-Van, N. A. @@aut@@ Kvashnin, A. N. @@aut@@ Martin, I. M. @@aut@@ Mizin, S. V. @@aut@@ Podgorny, A. I. @@aut@@ Stozhkov, Yu. I. @@aut@@ Turtelli, A. @@aut@@ |
| publishDateDaySort_date |
1994-03-01T00:00:00Z |
| hierarchy_top_id |
129367362 |
| dewey-sort |
3530 |
| id |
OLC2055372955 |
| 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">OLC2055372955</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230401104628.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s1994 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF02508588</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2055372955</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF02508588-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">16,13</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Bazilevskaya, G. A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1994</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">© Società Italiana di Fisica 1994</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bui-Van, N. A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kvashnin, A. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Martin, I. M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mizin, S. V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Podgorny, A. I.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stozhkov, Yu. I.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Turtelli, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Il Nuovo Cimento C</subfield><subfield code="d">Kluwer Academic Publishers, 1978</subfield><subfield code="g">17(1994), 2 vom: März, Seite 223-235</subfield><subfield code="w">(DE-627)129367362</subfield><subfield code="w">(DE-600)161886-6</subfield><subfield code="w">(DE-576)014741970</subfield><subfield code="x">1124-1896</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:17</subfield><subfield code="g">year:1994</subfield><subfield code="g">number:2</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:223-235</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF02508588</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-GEO</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-GGO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-GEO</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_11</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_40</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_130</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4103</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4155</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">17</subfield><subfield code="j">1994</subfield><subfield code="e">2</subfield><subfield code="c">03</subfield><subfield code="h">223-235</subfield></datafield></record></collection>
|
| author |
Bazilevskaya, G. A. |
| spellingShingle |
Bazilevskaya, G. A. ddc 530 ssgn 16,13 Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| authorStr |
Bazilevskaya, G. A. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)129367362 |
| format |
Article |
| dewey-ones |
530 - Physics |
| delete_txt_mv |
keep |
| author_role |
aut aut aut aut aut aut aut aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
1124-1896 |
| topic_title |
530 VZ 16,13 ssgn Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| topic |
ddc 530 ssgn 16,13 |
| topic_unstemmed |
ddc 530 ssgn 16,13 |
| topic_browse |
ddc 530 ssgn 16,13 |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| hierarchy_parent_title |
Il Nuovo Cimento C |
| hierarchy_parent_id |
129367362 |
| dewey-tens |
530 - Physics |
| hierarchy_top_title |
Il Nuovo Cimento C |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 |
| title |
Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| ctrlnum |
(DE-627)OLC2055372955 (DE-He213)BF02508588-p |
| title_full |
Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| author_sort |
Bazilevskaya, G. A. |
| journal |
Il Nuovo Cimento C |
| journalStr |
Il Nuovo Cimento C |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science |
| recordtype |
marc |
| publishDateSort |
1994 |
| contenttype_str_mv |
txt |
| container_start_page |
223 |
| author_browse |
Bazilevskaya, G. A. Bui-Van, N. A. Kvashnin, A. N. Martin, I. M. Mizin, S. V. Podgorny, A. I. Stozhkov, Yu. I. Turtelli, A. |
| container_volume |
17 |
| class |
530 VZ 16,13 ssgn |
| format_se |
Aufsätze |
| author-letter |
Bazilevskaya, G. A. |
| doi_str_mv |
10.1007/BF02508588 |
| dewey-full |
530 |
| title_sort |
time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| title_auth |
Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| abstract |
Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. © Società Italiana di Fisica 1994 |
| abstractGer |
Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. © Società Italiana di Fisica 1994 |
| abstract_unstemmed |
Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon. © Società Italiana di Fisica 1994 |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 |
| container_issue |
2 |
| title_short |
Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly |
| url |
https://doi.org/10.1007/BF02508588 |
| remote_bool |
false |
| author2 |
Bui-Van, N. A. Kvashnin, A. N. Martin, I. M. Mizin, S. V. Podgorny, A. I. Stozhkov, Yu. I. Turtelli, A. |
| author2Str |
Bui-Van, N. A. Kvashnin, A. N. Martin, I. M. Mizin, S. V. Podgorny, A. I. Stozhkov, Yu. I. Turtelli, A. |
| ppnlink |
129367362 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/BF02508588 |
| up_date |
2024-07-04T02:03:02.360Z |
| _version_ |
1803612148056719360 |
| 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">OLC2055372955</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230401104628.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s1994 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF02508588</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2055372955</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF02508588-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">16,13</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Bazilevskaya, G. A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Time fluctuations of charged and neutral cosmic-ray component fluxes as measured in the region of the brazilian magnetic anomaly</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1994</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">© Società Italiana di Fisica 1994</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Summary Measurements of charged particles, gamma emission and neutrons were fulfilled on balloon in the region of the Brazilian magnetic anomaly on 8 November 1991. The flight lasted approximately 18 hours, including 15 hours on the ceiling at the height of 32 km just during the beginning of the recovery phase of the moderate geomagnetic storm. The main conclusion from the analysis of the obtained experimental data is the following:a) the fluxes of charged and neutral particles were measured and are in agreement with the data of previous works for the close values of geomagnetic cut-off rigidity;b) no sporadic increases of charged- and neutral-particle fluxes were recorded;c) the pulsations of charged particles, gamma-rays and neutrons with characteristic time of ≈ 30 min were found. The sporadic pulsations of charged particles and gamma-rays with shorter periods were observed too. But later pulsations were absent in the neutron flux data. This points to the magnetospheric origin of the observed phenomenon.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bui-Van, N. A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kvashnin, A. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Martin, I. M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mizin, S. V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Podgorny, A. I.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stozhkov, Yu. I.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Turtelli, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Il Nuovo Cimento C</subfield><subfield code="d">Kluwer Academic Publishers, 1978</subfield><subfield code="g">17(1994), 2 vom: März, Seite 223-235</subfield><subfield code="w">(DE-627)129367362</subfield><subfield code="w">(DE-600)161886-6</subfield><subfield code="w">(DE-576)014741970</subfield><subfield code="x">1124-1896</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:17</subfield><subfield code="g">year:1994</subfield><subfield code="g">number:2</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:223-235</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF02508588</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-GEO</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-GGO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-GEO</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_11</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_40</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_130</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4103</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4155</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">17</subfield><subfield code="j">1994</subfield><subfield code="e">2</subfield><subfield code="c">03</subfield><subfield code="h">223-235</subfield></datafield></record></collection>
|
| score |
7.400429 |