Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004
We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Nickolaenko, A. P. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2014 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© Springer Science+Business Media New York 2014 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Radiophysics and quantum electronics - Springer US, 1969, 57(2014), 2 vom: Juli, Seite 125-140 |
|---|---|
| Übergeordnetes Werk: |
volume:57 ; year:2014 ; number:2 ; month:07 ; pages:125-140 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11141-014-9498-5 |
|---|
| Katalog-ID: |
OLC2063586233 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2063586233 | ||
| 003 | DE-627 | ||
| 005 | 20230504021607.0 | ||
| 007 | tu | ||
| 008 | 200820s2014 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/s11141-014-9498-5 |2 doi | |
| 035 | |a (DE-627)OLC2063586233 | ||
| 035 | |a (DE-He213)s11141-014-9498-5-p | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 530 |a 620 |q VZ |
| 100 | 1 | |a Nickolaenko, A. P. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 |
| 264 | 1 | |c 2014 | |
| 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 New York 2014 | ||
| 520 | |a We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. | ||
| 650 | 4 | |a Azimuth | |
| 650 | 4 | |a Poynting Vector | |
| 650 | 4 | |a Schumann Resonance | |
| 650 | 4 | |a Global Electric Circuit | |
| 650 | 4 | |a Bold Black Line | |
| 700 | 1 | |a Schekotov, A. Yu. |4 aut | |
| 700 | 1 | |a Hayakawa, M. |4 aut | |
| 700 | 1 | |a Hobara, Y. |4 aut | |
| 700 | 1 | |a Sátori, G. |4 aut | |
| 700 | 1 | |a Bor, J. |4 aut | |
| 700 | 1 | |a Neska, M. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Radiophysics and quantum electronics |d Springer US, 1969 |g 57(2014), 2 vom: Juli, Seite 125-140 |w (DE-627)130499560 |w (DE-600)760167-0 |w (DE-576)016080793 |x 0033-8443 |7 nnns |
| 773 | 1 | 8 | |g volume:57 |g year:2014 |g number:2 |g month:07 |g pages:125-140 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/s11141-014-9498-5 |z lizenzpflichtig |3 Volltext |
| 912 | |a GBV_USEFLAG_A | ||
| 912 | |a SYSFLAG_A | ||
| 912 | |a GBV_OLC | ||
| 912 | |a SSG-OLC-TEC | ||
| 912 | |a SSG-OLC-PHY | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_70 | ||
| 951 | |a AR | ||
| 952 | |d 57 |j 2014 |e 2 |c 07 |h 125-140 | ||
| author_variant |
a p n ap apn a y s ay ays m h mh y h yh g s gs j b jb m n mn |
|---|---|
| matchkey_str |
article:00338443:2014----::utpiteetooteltasetasdyhgmal |
| hierarchy_sort_str |
2014 |
| publishDate |
2014 |
| allfields |
10.1007/s11141-014-9498-5 doi (DE-627)OLC2063586233 (DE-He213)s11141-014-9498-5-p DE-627 ger DE-627 rakwb eng 530 620 VZ Nickolaenko, A. P. verfasserin aut Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. Azimuth Poynting Vector Schumann Resonance Global Electric Circuit Bold Black Line Schekotov, A. Yu. aut Hayakawa, M. aut Hobara, Y. aut Sátori, G. aut Bor, J. aut Neska, M. aut Enthalten in Radiophysics and quantum electronics Springer US, 1969 57(2014), 2 vom: Juli, Seite 125-140 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:57 year:2014 number:2 month:07 pages:125-140 https://doi.org/10.1007/s11141-014-9498-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 57 2014 2 07 125-140 |
| spelling |
10.1007/s11141-014-9498-5 doi (DE-627)OLC2063586233 (DE-He213)s11141-014-9498-5-p DE-627 ger DE-627 rakwb eng 530 620 VZ Nickolaenko, A. P. verfasserin aut Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. Azimuth Poynting Vector Schumann Resonance Global Electric Circuit Bold Black Line Schekotov, A. Yu. aut Hayakawa, M. aut Hobara, Y. aut Sátori, G. aut Bor, J. aut Neska, M. aut Enthalten in Radiophysics and quantum electronics Springer US, 1969 57(2014), 2 vom: Juli, Seite 125-140 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:57 year:2014 number:2 month:07 pages:125-140 https://doi.org/10.1007/s11141-014-9498-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 57 2014 2 07 125-140 |
| allfields_unstemmed |
10.1007/s11141-014-9498-5 doi (DE-627)OLC2063586233 (DE-He213)s11141-014-9498-5-p DE-627 ger DE-627 rakwb eng 530 620 VZ Nickolaenko, A. P. verfasserin aut Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. Azimuth Poynting Vector Schumann Resonance Global Electric Circuit Bold Black Line Schekotov, A. Yu. aut Hayakawa, M. aut Hobara, Y. aut Sátori, G. aut Bor, J. aut Neska, M. aut Enthalten in Radiophysics and quantum electronics Springer US, 1969 57(2014), 2 vom: Juli, Seite 125-140 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:57 year:2014 number:2 month:07 pages:125-140 https://doi.org/10.1007/s11141-014-9498-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 57 2014 2 07 125-140 |
| allfieldsGer |
10.1007/s11141-014-9498-5 doi (DE-627)OLC2063586233 (DE-He213)s11141-014-9498-5-p DE-627 ger DE-627 rakwb eng 530 620 VZ Nickolaenko, A. P. verfasserin aut Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. Azimuth Poynting Vector Schumann Resonance Global Electric Circuit Bold Black Line Schekotov, A. Yu. aut Hayakawa, M. aut Hobara, Y. aut Sátori, G. aut Bor, J. aut Neska, M. aut Enthalten in Radiophysics and quantum electronics Springer US, 1969 57(2014), 2 vom: Juli, Seite 125-140 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:57 year:2014 number:2 month:07 pages:125-140 https://doi.org/10.1007/s11141-014-9498-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 57 2014 2 07 125-140 |
| allfieldsSound |
10.1007/s11141-014-9498-5 doi (DE-627)OLC2063586233 (DE-He213)s11141-014-9498-5-p DE-627 ger DE-627 rakwb eng 530 620 VZ Nickolaenko, A. P. verfasserin aut Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. Azimuth Poynting Vector Schumann Resonance Global Electric Circuit Bold Black Line Schekotov, A. Yu. aut Hayakawa, M. aut Hobara, Y. aut Sátori, G. aut Bor, J. aut Neska, M. aut Enthalten in Radiophysics and quantum electronics Springer US, 1969 57(2014), 2 vom: Juli, Seite 125-140 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:57 year:2014 number:2 month:07 pages:125-140 https://doi.org/10.1007/s11141-014-9498-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 57 2014 2 07 125-140 |
| language |
English |
| source |
Enthalten in Radiophysics and quantum electronics 57(2014), 2 vom: Juli, Seite 125-140 volume:57 year:2014 number:2 month:07 pages:125-140 |
| sourceStr |
Enthalten in Radiophysics and quantum electronics 57(2014), 2 vom: Juli, Seite 125-140 volume:57 year:2014 number:2 month:07 pages:125-140 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Azimuth Poynting Vector Schumann Resonance Global Electric Circuit Bold Black Line |
| dewey-raw |
530 |
| isfreeaccess_bool |
false |
| container_title |
Radiophysics and quantum electronics |
| authorswithroles_txt_mv |
Nickolaenko, A. P. @@aut@@ Schekotov, A. Yu. @@aut@@ Hayakawa, M. @@aut@@ Hobara, Y. @@aut@@ Sátori, G. @@aut@@ Bor, J. @@aut@@ Neska, M. @@aut@@ |
| publishDateDaySort_date |
2014-07-01T00:00:00Z |
| hierarchy_top_id |
130499560 |
| dewey-sort |
3530 |
| id |
OLC2063586233 |
| 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">OLC2063586233</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504021607.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2014 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11141-014-9498-5</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2063586233</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11141-014-9498-5-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="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Nickolaenko, A. P.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2014</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 New York 2014</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Azimuth</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Poynting Vector</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Schumann Resonance</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Global Electric Circuit</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Bold Black Line</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Schekotov, A. Yu.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayakawa, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hobara, Y.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sátori, G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bor, J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Neska, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Radiophysics and quantum electronics</subfield><subfield code="d">Springer US, 1969</subfield><subfield code="g">57(2014), 2 vom: Juli, Seite 125-140</subfield><subfield code="w">(DE-627)130499560</subfield><subfield code="w">(DE-600)760167-0</subfield><subfield code="w">(DE-576)016080793</subfield><subfield code="x">0033-8443</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:57</subfield><subfield code="g">year:2014</subfield><subfield code="g">number:2</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:125-140</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s11141-014-9498-5</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-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</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_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">57</subfield><subfield code="j">2014</subfield><subfield code="e">2</subfield><subfield code="c">07</subfield><subfield code="h">125-140</subfield></datafield></record></collection>
|
| author |
Nickolaenko, A. P. |
| spellingShingle |
Nickolaenko, A. P. ddc 530 misc Azimuth misc Poynting Vector misc Schumann Resonance misc Global Electric Circuit misc Bold Black Line Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 |
| authorStr |
Nickolaenko, A. P. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)130499560 |
| format |
Article |
| dewey-ones |
530 - Physics 620 - Engineering & allied operations |
| delete_txt_mv |
keep |
| author_role |
aut aut aut aut aut aut aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0033-8443 |
| topic_title |
530 620 VZ Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 Azimuth Poynting Vector Schumann Resonance Global Electric Circuit Bold Black Line |
| topic |
ddc 530 misc Azimuth misc Poynting Vector misc Schumann Resonance misc Global Electric Circuit misc Bold Black Line |
| topic_unstemmed |
ddc 530 misc Azimuth misc Poynting Vector misc Schumann Resonance misc Global Electric Circuit misc Bold Black Line |
| topic_browse |
ddc 530 misc Azimuth misc Poynting Vector misc Schumann Resonance misc Global Electric Circuit misc Bold Black Line |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| hierarchy_parent_title |
Radiophysics and quantum electronics |
| hierarchy_parent_id |
130499560 |
| dewey-tens |
530 - Physics 620 - Engineering |
| hierarchy_top_title |
Radiophysics and quantum electronics |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 |
| title |
Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 |
| ctrlnum |
(DE-627)OLC2063586233 (DE-He213)s11141-014-9498-5-p |
| title_full |
Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 |
| author_sort |
Nickolaenko, A. P. |
| journal |
Radiophysics and quantum electronics |
| journalStr |
Radiophysics and quantum electronics |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science 600 - Technology |
| recordtype |
marc |
| publishDateSort |
2014 |
| contenttype_str_mv |
txt |
| container_start_page |
125 |
| author_browse |
Nickolaenko, A. P. Schekotov, A. Yu. Hayakawa, M. Hobara, Y. Sátori, G. Bor, J. Neska, M. |
| container_volume |
57 |
| class |
530 620 VZ |
| format_se |
Aufsätze |
| author-letter |
Nickolaenko, A. P. |
| doi_str_mv |
10.1007/s11141-014-9498-5 |
| dewey-full |
530 620 |
| title_sort |
multi-point detection of the elf transient caused by the gamma flare of december 27, 2004 |
| title_auth |
Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 |
| abstract |
We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. © Springer Science+Business Media New York 2014 |
| abstractGer |
We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. © Springer Science+Business Media New York 2014 |
| abstract_unstemmed |
We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare. © Springer Science+Business Media New York 2014 |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 |
| container_issue |
2 |
| title_short |
Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004 |
| url |
https://doi.org/10.1007/s11141-014-9498-5 |
| remote_bool |
false |
| author2 |
Schekotov, A. Yu Hayakawa, M. Hobara, Y. Sátori, G. Bor, J. Neska, M. |
| author2Str |
Schekotov, A. Yu Hayakawa, M. Hobara, Y. Sátori, G. Bor, J. Neska, M. |
| ppnlink |
130499560 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/s11141-014-9498-5 |
| up_date |
2024-07-03T19:30:49.728Z |
| _version_ |
1803587472308830208 |
| 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">OLC2063586233</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504021607.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2014 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11141-014-9498-5</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2063586233</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11141-014-9498-5-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="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Nickolaenko, A. P.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Multi-Point Detection of the Elf Transient Caused by the Gamma Flare of December 27, 2004</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2014</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 New York 2014</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present the experimental records of the radio pulse related to the gamma burst that took place on December 27, 2004. The records, which are synchronized by GPS time marks, were obtained in the observatories at Moshiri and Onagawa (Japan), Esrange (Sweden), Karimshino (Kamchatka, Russia), Nagycenk (Hungary), and Hornsund (Polish Polar Station Spitzbergen). The data demonstrate exceptional similarity and contain characteristic pulses that correspond to the time of gamma-ray arrival. Processing of the signals shows that along with the time match, the following modeling predictions are confirmed: radio pulses contain a signal at the main frequency of the Schumann resonance, the field source has positive polarity (the current is directed from the ionosphere towards the Earth), the polarization of the horizontal magnetic field of the radio wave is almost linear, and the directions towards the source indicate the epicenter of the gamma-quanta flux collision with the ionosphere. These properties correspond to the concept of the parametric electromagnetic pulse that is produced due to a significant change in the current in the global electric circuit, which is caused by a cosmic gamma-ray flare.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Azimuth</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Poynting Vector</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Schumann Resonance</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Global Electric Circuit</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Bold Black Line</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Schekotov, A. Yu.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayakawa, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hobara, Y.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sátori, G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bor, J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Neska, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Radiophysics and quantum electronics</subfield><subfield code="d">Springer US, 1969</subfield><subfield code="g">57(2014), 2 vom: Juli, Seite 125-140</subfield><subfield code="w">(DE-627)130499560</subfield><subfield code="w">(DE-600)760167-0</subfield><subfield code="w">(DE-576)016080793</subfield><subfield code="x">0033-8443</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:57</subfield><subfield code="g">year:2014</subfield><subfield code="g">number:2</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:125-140</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s11141-014-9498-5</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-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</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_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">57</subfield><subfield code="j">2014</subfield><subfield code="e">2</subfield><subfield code="c">07</subfield><subfield code="h">125-140</subfield></datafield></record></collection>
|
| score |
7.399496 |