Decameter U-burst Harmonic Pair from a High Loop
Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Dorovskyy, V. V. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2014 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© Springer Science+Business Media Dordrecht 2014 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Solar physics - Springer Netherlands, 1967, 290(2014), 1 vom: 21. Okt., Seite 181-192 |
|---|---|
| Übergeordnetes Werk: |
volume:290 ; year:2014 ; number:1 ; day:21 ; month:10 ; pages:181-192 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11207-014-0615-6 |
|---|
| Katalog-ID: |
OLC2033617572 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2033617572 | ||
| 003 | DE-627 | ||
| 005 | 20230504050007.0 | ||
| 007 | tu | ||
| 008 | 200819s2014 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/s11207-014-0615-6 |2 doi | |
| 035 | |a (DE-627)OLC2033617572 | ||
| 035 | |a (DE-He213)s11207-014-0615-6-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 Dorovskyy, V. V. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Decameter U-burst Harmonic Pair from a High Loop |
| 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 Dordrecht 2014 | ||
| 520 | |a Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. | ||
| 650 | 4 | |a Corona, radio emission | |
| 650 | 4 | |a Corona, structures | |
| 650 | 4 | |a Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) | |
| 650 | 4 | |a Radio bursts, type U | |
| 650 | 4 | |a Radio bursts, harmonic pairs | |
| 700 | 1 | |a Melnik, V. N. |4 aut | |
| 700 | 1 | |a Konovalenko, A. A. |4 aut | |
| 700 | 1 | |a Bubnov, I. N. |4 aut | |
| 700 | 1 | |a Gridin, A. A. |4 aut | |
| 700 | 1 | |a Shevchuk, N. V. |4 aut | |
| 700 | 1 | |a Rucker, H. O. |4 aut | |
| 700 | 1 | |a Poedts, S. |4 aut | |
| 700 | 1 | |a Panchenko, M. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Solar physics |d Springer Netherlands, 1967 |g 290(2014), 1 vom: 21. Okt., Seite 181-192 |w (DE-627)129856010 |w (DE-600)281593-X |w (DE-576)015160033 |x 0038-0938 |7 nnns |
| 773 | 1 | 8 | |g volume:290 |g year:2014 |g number:1 |g day:21 |g month:10 |g pages:181-192 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/s11207-014-0615-6 |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 290 |j 2014 |e 1 |b 21 |c 10 |h 181-192 | ||
| author_variant |
v v d vv vvd v n m vn vnm a a k aa aak i n b in inb a a g aa aag n v s nv nvs h o r ho hor s p sp m p mp |
|---|---|
| matchkey_str |
article:00380938:2014----::eaeeuushroipifo |
| hierarchy_sort_str |
2014 |
| publishDate |
2014 |
| allfields |
10.1007/s11207-014-0615-6 doi (DE-627)OLC2033617572 (DE-He213)s11207-014-0615-6-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Dorovskyy, V. V. verfasserin aut Decameter U-burst Harmonic Pair from a High Loop 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. Corona, radio emission Corona, structures Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) Radio bursts, type U Radio bursts, harmonic pairs Melnik, V. N. aut Konovalenko, A. A. aut Bubnov, I. N. aut Gridin, A. A. aut Shevchuk, N. V. aut Rucker, H. O. aut Poedts, S. aut Panchenko, M. aut Enthalten in Solar physics Springer Netherlands, 1967 290(2014), 1 vom: 21. Okt., Seite 181-192 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:290 year:2014 number:1 day:21 month:10 pages:181-192 https://doi.org/10.1007/s11207-014-0615-6 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 290 2014 1 21 10 181-192 |
| spelling |
10.1007/s11207-014-0615-6 doi (DE-627)OLC2033617572 (DE-He213)s11207-014-0615-6-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Dorovskyy, V. V. verfasserin aut Decameter U-burst Harmonic Pair from a High Loop 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. Corona, radio emission Corona, structures Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) Radio bursts, type U Radio bursts, harmonic pairs Melnik, V. N. aut Konovalenko, A. A. aut Bubnov, I. N. aut Gridin, A. A. aut Shevchuk, N. V. aut Rucker, H. O. aut Poedts, S. aut Panchenko, M. aut Enthalten in Solar physics Springer Netherlands, 1967 290(2014), 1 vom: 21. Okt., Seite 181-192 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:290 year:2014 number:1 day:21 month:10 pages:181-192 https://doi.org/10.1007/s11207-014-0615-6 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 290 2014 1 21 10 181-192 |
| allfields_unstemmed |
10.1007/s11207-014-0615-6 doi (DE-627)OLC2033617572 (DE-He213)s11207-014-0615-6-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Dorovskyy, V. V. verfasserin aut Decameter U-burst Harmonic Pair from a High Loop 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. Corona, radio emission Corona, structures Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) Radio bursts, type U Radio bursts, harmonic pairs Melnik, V. N. aut Konovalenko, A. A. aut Bubnov, I. N. aut Gridin, A. A. aut Shevchuk, N. V. aut Rucker, H. O. aut Poedts, S. aut Panchenko, M. aut Enthalten in Solar physics Springer Netherlands, 1967 290(2014), 1 vom: 21. Okt., Seite 181-192 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:290 year:2014 number:1 day:21 month:10 pages:181-192 https://doi.org/10.1007/s11207-014-0615-6 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 290 2014 1 21 10 181-192 |
| allfieldsGer |
10.1007/s11207-014-0615-6 doi (DE-627)OLC2033617572 (DE-He213)s11207-014-0615-6-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Dorovskyy, V. V. verfasserin aut Decameter U-burst Harmonic Pair from a High Loop 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. Corona, radio emission Corona, structures Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) Radio bursts, type U Radio bursts, harmonic pairs Melnik, V. N. aut Konovalenko, A. A. aut Bubnov, I. N. aut Gridin, A. A. aut Shevchuk, N. V. aut Rucker, H. O. aut Poedts, S. aut Panchenko, M. aut Enthalten in Solar physics Springer Netherlands, 1967 290(2014), 1 vom: 21. Okt., Seite 181-192 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:290 year:2014 number:1 day:21 month:10 pages:181-192 https://doi.org/10.1007/s11207-014-0615-6 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 290 2014 1 21 10 181-192 |
| allfieldsSound |
10.1007/s11207-014-0615-6 doi (DE-627)OLC2033617572 (DE-He213)s11207-014-0615-6-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Dorovskyy, V. V. verfasserin aut Decameter U-burst Harmonic Pair from a High Loop 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. Corona, radio emission Corona, structures Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) Radio bursts, type U Radio bursts, harmonic pairs Melnik, V. N. aut Konovalenko, A. A. aut Bubnov, I. N. aut Gridin, A. A. aut Shevchuk, N. V. aut Rucker, H. O. aut Poedts, S. aut Panchenko, M. aut Enthalten in Solar physics Springer Netherlands, 1967 290(2014), 1 vom: 21. Okt., Seite 181-192 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:290 year:2014 number:1 day:21 month:10 pages:181-192 https://doi.org/10.1007/s11207-014-0615-6 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 290 2014 1 21 10 181-192 |
| language |
English |
| source |
Enthalten in Solar physics 290(2014), 1 vom: 21. Okt., Seite 181-192 volume:290 year:2014 number:1 day:21 month:10 pages:181-192 |
| sourceStr |
Enthalten in Solar physics 290(2014), 1 vom: 21. Okt., Seite 181-192 volume:290 year:2014 number:1 day:21 month:10 pages:181-192 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Corona, radio emission Corona, structures Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) Radio bursts, type U Radio bursts, harmonic pairs |
| dewey-raw |
530 |
| isfreeaccess_bool |
false |
| container_title |
Solar physics |
| authorswithroles_txt_mv |
Dorovskyy, V. V. @@aut@@ Melnik, V. N. @@aut@@ Konovalenko, A. A. @@aut@@ Bubnov, I. N. @@aut@@ Gridin, A. A. @@aut@@ Shevchuk, N. V. @@aut@@ Rucker, H. O. @@aut@@ Poedts, S. @@aut@@ Panchenko, M. @@aut@@ |
| publishDateDaySort_date |
2014-10-21T00:00:00Z |
| hierarchy_top_id |
129856010 |
| dewey-sort |
3530 |
| id |
OLC2033617572 |
| 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">OLC2033617572</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504050007.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2014 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11207-014-0615-6</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033617572</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11207-014-0615-6-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">Dorovskyy, V. V.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Decameter U-burst Harmonic Pair from a High Loop</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 Dordrecht 2014</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Corona, radio emission</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Corona, structures</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio bursts, meter-wavelengths and longer (m, dkm, hm, km)</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio bursts, type U</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio bursts, harmonic pairs</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Melnik, V. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Konovalenko, A. A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bubnov, I. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Gridin, A. A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shevchuk, N. V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rucker, H. O.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Poedts, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Panchenko, M.</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">290(2014), 1 vom: 21. Okt., Seite 181-192</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:290</subfield><subfield code="g">year:2014</subfield><subfield code="g">number:1</subfield><subfield code="g">day:21</subfield><subfield code="g">month:10</subfield><subfield code="g">pages:181-192</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s11207-014-0615-6</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">290</subfield><subfield code="j">2014</subfield><subfield code="e">1</subfield><subfield code="b">21</subfield><subfield code="c">10</subfield><subfield code="h">181-192</subfield></datafield></record></collection>
|
| author |
Dorovskyy, V. V. |
| spellingShingle |
Dorovskyy, V. V. ddc 530 ssgn 16,12 misc Corona, radio emission misc Corona, structures misc Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) misc Radio bursts, type U misc Radio bursts, harmonic pairs Decameter U-burst Harmonic Pair from a High Loop |
| authorStr |
Dorovskyy, V. V. |
| 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 aut aut aut aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0038-0938 |
| topic_title |
530 VZ 16,12 ssgn Decameter U-burst Harmonic Pair from a High Loop Corona, radio emission Corona, structures Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) Radio bursts, type U Radio bursts, harmonic pairs |
| topic |
ddc 530 ssgn 16,12 misc Corona, radio emission misc Corona, structures misc Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) misc Radio bursts, type U misc Radio bursts, harmonic pairs |
| topic_unstemmed |
ddc 530 ssgn 16,12 misc Corona, radio emission misc Corona, structures misc Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) misc Radio bursts, type U misc Radio bursts, harmonic pairs |
| topic_browse |
ddc 530 ssgn 16,12 misc Corona, radio emission misc Corona, structures misc Radio bursts, meter-wavelengths and longer (m, dkm, hm, km) misc Radio bursts, type U misc Radio bursts, harmonic pairs |
| 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 |
Decameter U-burst Harmonic Pair from a High Loop |
| ctrlnum |
(DE-627)OLC2033617572 (DE-He213)s11207-014-0615-6-p |
| title_full |
Decameter U-burst Harmonic Pair from a High Loop |
| author_sort |
Dorovskyy, V. V. |
| journal |
Solar physics |
| journalStr |
Solar physics |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science |
| recordtype |
marc |
| publishDateSort |
2014 |
| contenttype_str_mv |
txt |
| container_start_page |
181 |
| author_browse |
Dorovskyy, V. V. Melnik, V. N. Konovalenko, A. A. Bubnov, I. N. Gridin, A. A. Shevchuk, N. V. Rucker, H. O. Poedts, S. Panchenko, M. |
| container_volume |
290 |
| class |
530 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Dorovskyy, V. V. |
| doi_str_mv |
10.1007/s11207-014-0615-6 |
| dewey-full |
530 |
| title_sort |
decameter u-burst harmonic pair from a high loop |
| title_auth |
Decameter U-burst Harmonic Pair from a High Loop |
| abstract |
Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. © Springer Science+Business Media Dordrecht 2014 |
| abstractGer |
Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. © Springer Science+Business Media Dordrecht 2014 |
| abstract_unstemmed |
Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies. © Springer Science+Business Media Dordrecht 2014 |
| 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 |
1 |
| title_short |
Decameter U-burst Harmonic Pair from a High Loop |
| url |
https://doi.org/10.1007/s11207-014-0615-6 |
| remote_bool |
false |
| author2 |
Melnik, V. N. Konovalenko, A. A. Bubnov, I. N. Gridin, A. A. Shevchuk, N. V. Rucker, H. O. Poedts, S. Panchenko, M. |
| author2Str |
Melnik, V. N. Konovalenko, A. A. Bubnov, I. N. Gridin, A. A. Shevchuk, N. V. Rucker, H. O. Poedts, S. Panchenko, M. |
| ppnlink |
129856010 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/s11207-014-0615-6 |
| up_date |
2024-07-03T17:43:41.474Z |
| _version_ |
1803580731791769601 |
| 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">OLC2033617572</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504050007.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2014 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11207-014-0615-6</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033617572</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11207-014-0615-6-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">Dorovskyy, V. V.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Decameter U-burst Harmonic Pair from a High Loop</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 Dordrecht 2014</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The results of the first observations of solar sporadic radio emission within 10 – 70 MHz by the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in such a wide range of frequencies considerably facilitate the registration of harmonic pairs. The solar U-burst harmonic pair observed on 8 August 2012 is analyzed. The burst key features were determined. Among them, the time delay between the fundamental and harmonic emissions was of special interest. The fundamental emission was delayed for 7 s with respect to the harmonic emission. A model for explaining the occurrence of such a delay is proposed, in which the emission source is located inside a magnetic loop containing plasma of increased density. In this case, the delay appears due to the difference in group velocities of electromagnetic waves at the fundamental and the harmonic frequencies.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Corona, radio emission</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Corona, structures</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio bursts, meter-wavelengths and longer (m, dkm, hm, km)</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio bursts, type U</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio bursts, harmonic pairs</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Melnik, V. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Konovalenko, A. A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bubnov, I. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Gridin, A. A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shevchuk, N. V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rucker, H. O.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Poedts, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Panchenko, M.</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">290(2014), 1 vom: 21. Okt., Seite 181-192</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:290</subfield><subfield code="g">year:2014</subfield><subfield code="g">number:1</subfield><subfield code="g">day:21</subfield><subfield code="g">month:10</subfield><subfield code="g">pages:181-192</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s11207-014-0615-6</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">290</subfield><subfield code="j">2014</subfield><subfield code="e">1</subfield><subfield code="b">21</subfield><subfield code="c">10</subfield><subfield code="h">181-192</subfield></datafield></record></collection>
|
| score |
7.4011803 |