Nonlinear distribution of the sunspot magnetic field during the solar maximum
Using the standard solar w-dynamo equations we formulate appropriate initial and boundary conditions at the moment when the toroidal component is maximum, so that we obtain the toroidal magnetic field component as a function of the solar latitude. We found a new non-homogeneous distribution for the...
Saved in:
| Published in | Advances in space research Vol. 32; no. 6; pp. 1175 - 1180 |
|---|---|
| Main Authors | , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Elsevier Ltd
01.09.2003
|
| Online Access | Get full text |
Cover
Loading…
| Abstract | Using the standard solar w-dynamo equations we formulate appropriate initial and boundary conditions at the moment when the toroidal component is maximum, so that we obtain the toroidal magnetic field component as a function of the solar latitude. We found a new non-homogeneous distribution for the toroidal component along the latitude (〈
ΔB
θ
/
Δθ〉) given by 7G/
degree, 24G/
degree and 34G/
degree for the respectiives latitudes ranges of 10°-15°, 16°-18° and 19°-25°) and this nonhomogenous decay rate is statistically confirmed through a chi-square analysis of the Mt. Wilson Sunspot data for two solar cycles. Based on this result one can expect the most energetic magnetic eruptive phenomena to be, in average, nonlinearly concentrated at latitudes ranging from 10 to 25 degrees in both hemispheres. |
|---|---|
| AbstractList | Using the standard solar w-dynamo equations we formulate appropriate initial and boundary conditions at the moment when the toroidal component is maximum, so that we obtain the toroidal magnetic field component as a function of the solar latitude. We found a new non-homogeneous distribution for the toroidal component along the latitude (〈
ΔB
θ
/
Δθ〉) given by 7G/
degree, 24G/
degree and 34G/
degree for the respectiives latitudes ranges of 10°-15°, 16°-18° and 19°-25°) and this nonhomogenous decay rate is statistically confirmed through a chi-square analysis of the Mt. Wilson Sunspot data for two solar cycles. Based on this result one can expect the most energetic magnetic eruptive phenomena to be, in average, nonlinearly concentrated at latitudes ranging from 10 to 25 degrees in both hemispheres. Using the standard solar w-dynamo equations we formulate appropriate initial and boundary conditions at the moment when the toroidal component is maximum, so that we obtain the toroidal magnetic field component as a function of the solar latitude. We found a new non-homogeneous distribution for the toroidal component along the latitude (<[Delta]B sub( theta theta])/[Delta] theta theta]>) given by 7G/degree, 24G/degree and 34G/degree for the respectiives latitudes ranges of 10 degree - 15 degree , 16 degree -18 degree and 19 degree -25 degree ) and this nonhomogenous decay rate is statistically confirmed through a chi-square analysis of the Mt. Wilson Sunspot data for two solar cycles. Based on this result one can expect the most energetic magnetic eruptive phenomena to be, in average, nonlinearly concentrated at latitudes ranging from 10 to 25 degrees in both hemispheres. Using the standard solar w-dynamo equations we formulate appropriate initial and boundary conditions at the moment when the toroidal component is maximum, so that we obtain the toroidal magnetic field component as a function of the solar latitude. We found a new non-homogeneous distribution for the toroidal component along the latitude ( < Delta B sub Theta theta]/ Delta Theta theta] > ) given by 7G /degree, 24G/degree and 34G/degree for the respectiives latitudes ranges of 10 - 15 , 16 -18 and 19 -25 ) and this nonhomogenous decay rate is statistically confirmed through a chi-square analysis of the Mt. Wilson Sunspot data for two solar cycles. Based on this result one can expect the most energetic magnetic eruptive phenomena to be, in average, nonlinearly concentrated at latitudes ranging from 10 to 25 degrees in both hemispheres. |
| Author | Vijaykumar, Nandamudi L. Rosa, Reinaldo R. Gonzalez-Machado, Encarnacion A.M. Boechat-Roberty, Heloisa M. Sawant, Hanumant S. |
| Author_xml | – sequence: 1 givenname: Reinaldo R. surname: Rosa fullname: Rosa, Reinaldo R. email: reinaldo@lac.inpe.br organization: Lab for Computing and Applied Mathematics (LAC), National Institute for Space Research-INPE, C.P. 515, 12201-970, São José dos Campos, Brazil – sequence: 2 givenname: Encarnacion A.M. surname: Gonzalez-Machado fullname: Gonzalez-Machado, Encarnacion A.M. organization: Department of Astronomy (OV), Universidade Federal do Rio de Janeiro, Brazil – sequence: 3 givenname: Heloisa M. surname: Boechat-Roberty fullname: Boechat-Roberty, Heloisa M. organization: Department of Astronomy (OV), Universidade Federal do Rio de Janeiro, Brazil – sequence: 4 givenname: Nandamudi L. surname: Vijaykumar fullname: Vijaykumar, Nandamudi L. organization: Lab for Computing and Applied Mathematics (LAC), National Institute for Space Research-INPE, C.P. 515, 12201-970, São José dos Campos, Brazil – sequence: 5 givenname: Hanumant S. surname: Sawant fullname: Sawant, Hanumant S. organization: Astrophysics Division (DAS) - INPE, Brazil |
| BookMark | eNqFkEtLxDAUhYOM4MzoTxC6El1U82iTZiUy-AIfC3UdMsntGGmTMWlF_72dqbid1eXAdw7cb4YmPnhA6Jjgc4IJv3jBVLCcECFOMTvDmNEyl3toSiohcyKLaoKm_8gBmqX0gTGhQuApenwKvnEedMysS110y75zwWehzrp3yFLv0zp0WatXHjpnstpBYzPbR-dXIxGaodvqb9f27SHar3WT4OjvztHbzfXr4i5_eL69X1w95IZx2eWaUk6WFEtrQRrDSlNSSwsLdQ1cc211YY3gwspCVkOouDEY-BLXrCCCFWyOTsbddQyfPaROtS4ZaBrtIfRJUVFVkpZkJ0gqXGBJNmA5giaGlCLUah1dq-OPIlhtLKutZbVRqDBTW8tKDr3LsQfDu18OokrGgTdgXQTTKRvcjoVfGq-HEQ |
| CitedBy_id | crossref_primary_10_15406_paij_2023_07_00283 |
| Cites_doi | 10.1086/149943 10.1002/1521-3994(200208)323:3/4<411::AID-ASNA411>3.0.CO;2-H 10.1086/146010 10.1051/0004-6361:20021224 10.1086/175536 10.1007/BF00148202 10.1002/asna.19692910201 10.1007/BF00148198 10.1007/BF00151634 10.1086/304484 10.1086/147060 10.1007/BF00146532 10.1007/BF00158425 10.1086/151840 10.1086/190355 10.1051/0004-6361:20020590 10.1086/306748 10.1086/322410 10.1002/1521-3994(200208)323:3/4<432::AID-ASNA432>3.0.CO;2-5 10.1086/304546 10.1007/BF00206186 10.1086/153940 |
| ContentType | Journal Article |
| Copyright | 2003 |
| Copyright_xml | – notice: 2003 |
| DBID | AAYXX CITATION 7TG KL. 8FD H8D L7M |
| DOI | 10.1016/S0273-1177(03)00325-9 |
| DatabaseName | CrossRef Meteorological & Geoastrophysical Abstracts Meteorological & Geoastrophysical Abstracts - Academic Technology Research Database Aerospace Database Advanced Technologies Database with Aerospace |
| DatabaseTitle | CrossRef Meteorological & Geoastrophysical Abstracts - Academic Meteorological & Geoastrophysical Abstracts Technology Research Database Aerospace Database Advanced Technologies Database with Aerospace |
| DatabaseTitleList | Meteorological & Geoastrophysical Abstracts - Academic Technology Research Database |
| DeliveryMethod | fulltext_linktorsrc |
| Discipline | Engineering Astronomy & Astrophysics Physics |
| EISSN | 1879-1948 |
| EndPage | 1180 |
| ExternalDocumentID | 10_1016_S0273_1177_03_00325_9 S0273117703003259 |
| GroupedDBID | --K --M -~X .~1 0R~ 1B1 1RT 1~. 1~5 23M 4.4 457 4G. 53G 5GY 5VS 7-5 71M 8P~ 9JN AACTN AAEDT AAEDW AAIAV AAIKJ AAKOC AALRI AAOAW AAQFI AAQXK AAXUO ABFNM ABJNI ABMAC ABNEU ABQEM ABQYD ABTAH ABXDB ABYKQ ACDAQ ACFVG ACGFS ACLVX ACNNM ACRLP ACSBN ADBBV ADEZE ADMUD AEBSH AEKER AENEX AFKWA AFTJW AGHFR AGUBO AGYEJ AHHHB AI. AIEXJ AIKHN AITUG AIVDX AJBFU AJOXV ALMA_UNASSIGNED_HOLDINGS AMFUW AMRAJ ASPBG ATOGT AVWKF AXJTR AZFZN BKOJK BLXMC CS3 EBS EFJIC EFLBG EJD EO8 EO9 EP2 EP3 F5P FDB FEDTE FGOYB FIRID FNPLU FYGXN G-2 G-Q GBLVA HMA HME HVGLF HX~ HZ~ IHE IMUCA J1W KOM LY3 LZ4 M41 MO0 N9A O-L O9- OAUVE OGIMB OZT P-8 P-9 P2P PC. Q38 R2- RIG ROL RPZ SDF SDG SEP SES SEW SHN SPC SPCBC SSE SSQ SSZ T5K T9H UHS VH1 VOH WUQ ZMT ZY4 ~02 ~G- AAXKI AAYXX AFJKZ AKRWK CITATION 7TG KL. 8FD H8D L7M |
| ID | FETCH-LOGICAL-c369t-a2261b209dde9cc35c52d24deffe6a6ada4dc767d9498da486cc0e6b0f3417343 |
| IEDL.DBID | .~1 |
| ISSN | 0273-1177 |
| IngestDate | Sat Oct 05 06:18:13 EDT 2024 Fri Oct 25 03:55:02 EDT 2024 Thu Sep 26 18:52:22 EDT 2024 Fri Feb 23 02:23:38 EST 2024 |
| IsPeerReviewed | true |
| IsScholarly | true |
| Issue | 6 |
| Language | English |
| LinkModel | DirectLink |
| MergedId | FETCHMERGED-LOGICAL-c369t-a2261b209dde9cc35c52d24deffe6a6ada4dc767d9498da486cc0e6b0f3417343 |
| Notes | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
| PQID | 18040911 |
| PQPubID | 23462 |
| PageCount | 6 |
| ParticipantIDs | proquest_miscellaneous_27889251 proquest_miscellaneous_18040911 crossref_primary_10_1016_S0273_1177_03_00325_9 elsevier_sciencedirect_doi_10_1016_S0273_1177_03_00325_9 |
| PublicationCentury | 2000 |
| PublicationDate | 20030901 |
| PublicationDateYYYYMMDD | 2003-09-01 |
| PublicationDate_xml | – month: 09 year: 2003 text: 20030901 day: 01 |
| PublicationDecade | 2000 |
| PublicationTitle | Advances in space research |
| PublicationYear | 2003 |
| Publisher | Elsevier Ltd |
| Publisher_xml | – name: Elsevier Ltd |
| References | Wilson (BIB25) 1991; 127 Subramanian (BIB20) 2002; V. 12 Parker (BIB15) 1987; 110 Yoshimura (BIB28) 1975; 201 MacGregor, Charbonneau (BIB11) 1997; 486 Durney (BIB9) 1997; 486 Dikpati, Gilman (BIB7) 1999; 512 Wilson (BIB24) 1987; 110 Yoshimura (BIB26) 1972; 178 Rudiger, Elstner (BIB16) 2002; 323 Babcock (BIB2) 1961; 133 Norusis (BIB12) 1985 Bonanno, Elstner, Rudiger, Belvedere (BIB4) 2002; 390 Ossendrijver, Stix, Brandenburg, Rudiger (BIB13) 2002; 394 Covas, Tworkowski, Brandenburg, Tavakol (BIB6) 1997; 317 Tobias, Proctor, Knobloch (BIB23) 1997; 318 Ruzmaikin (BIB17) 1985; 100 Ruzmaikin (BIB18) 1991; 131 Yoshimura (BIB29) 1976; 50 Brandenburg, Dobler (BIB3) 2002 Choudhuri, Schussler, Dikpati (BIB5) 1995; 303 Tao, Du, Rosner, Cattaneo (BIB22) 1995; 443 Steenbeck, Krause (BIB21) 1969; 291 Alfven (BIB1) 1981 Parker (BIB14) 1955; 121 Dikpati, Gilman (BIB8) 2001; 559 Shmitt (BIB19) 1984 Leighton (BIB10) 1969; 156 Zirin (BIB30) 1988 Yoshimura (BIB27) 1975; 29 Parker (10.1016/S0273-1177(03)00325-9_BIB14) 1955; 121 Subramanian (10.1016/S0273-1177(03)00325-9_BIB20) 2002; V. 12 Durney (10.1016/S0273-1177(03)00325-9_BIB9) 1997; 486 Ruzmaikin (10.1016/S0273-1177(03)00325-9_BIB18) 1991; 131 Ruzmaikin (10.1016/S0273-1177(03)00325-9_BIB17) 1985; 100 Ossendrijver (10.1016/S0273-1177(03)00325-9_BIB13) 2002; 394 Choudhuri (10.1016/S0273-1177(03)00325-9_BIB5) 1995; 303 Dikpati (10.1016/S0273-1177(03)00325-9_BIB8) 2001; 559 Dikpati (10.1016/S0273-1177(03)00325-9_BIB7) 1999; 512 Parker (10.1016/S0273-1177(03)00325-9_BIB15) 1987; 110 Tobias (10.1016/S0273-1177(03)00325-9_BIB23) 1997; 318 Zirin (10.1016/S0273-1177(03)00325-9_BIB30) 1988 Norusis (10.1016/S0273-1177(03)00325-9_BIB12) 1985 Babcock (10.1016/S0273-1177(03)00325-9_BIB2) 1961; 133 Brandenburg (10.1016/S0273-1177(03)00325-9_BIB3) 2002 Leighton (10.1016/S0273-1177(03)00325-9_BIB10) 1969; 156 Wilson (10.1016/S0273-1177(03)00325-9_BIB25) 1991; 127 Yoshimura (10.1016/S0273-1177(03)00325-9_BIB27) 1975; 29 Bonanno (10.1016/S0273-1177(03)00325-9_BIB4) 2002; 390 MacGregor (10.1016/S0273-1177(03)00325-9_BIB11) 1997; 486 Covas (10.1016/S0273-1177(03)00325-9_BIB6) 1997; 317 Yoshimura (10.1016/S0273-1177(03)00325-9_BIB29) 1976; 50 Yoshimura (10.1016/S0273-1177(03)00325-9_BIB26) 1972; 178 Wilson (10.1016/S0273-1177(03)00325-9_BIB24) 1987; 110 Yoshimura (10.1016/S0273-1177(03)00325-9_BIB28) 1975; 201 Steenbeck (10.1016/S0273-1177(03)00325-9_BIB21) 1969; 291 Tao (10.1016/S0273-1177(03)00325-9_BIB22) 1995; 443 Rudiger (10.1016/S0273-1177(03)00325-9_BIB16) 2002; 323 Alfven (10.1016/S0273-1177(03)00325-9_BIB1) 1981 Shmitt (10.1016/S0273-1177(03)00325-9_BIB19) 1984 |
| References_xml | – volume: 317 start-page: 610 year: 1997 ident: BIB6 article-title: Dynamos with different formulations of a dynamic alpha-effect publication-title: Astron. Astrophys. contributor: fullname: Tavakol – volume: 156 start-page: 1 year: 1969 ident: BIB10 article-title: A Magneto-Kinematic Model of the Solar Cycle publication-title: Ap. J. contributor: fullname: Leighton – volume: 512 start-page: 417 year: 1999 ident: BIB7 article-title: Joint Instability of Latitudinal Differential Rotation and Concentrated Toroidal Fields below the Solar Convection Zone publication-title: Ap. J. contributor: fullname: Gilman – volume: 133 start-page: 572 year: 1961 ident: BIB2 article-title: The topology of the Sun's magnetic field and the 22-year cycle publication-title: Ap. J. contributor: fullname: Babcock – volume: 323 start-page: 432 year: 2002 end-page: 435 ident: BIB16 article-title: Is the Butterfly diagram due to meridional motions? publication-title: Astr. Nach. contributor: fullname: Elstner – year: 2002 ident: BIB3 article-title: Solar and stellar dynamos — latest developments publication-title: Astron. Nachr. contributor: fullname: Dobler – volume: 100 start-page: 125 year: 1985 ident: BIB17 article-title: The solar dynamo publication-title: Solar Phys. contributor: fullname: Ruzmaikin – start-page: 223 year: 1984 end-page: 224 ident: BIB19 article-title: Dynamo action of magnetostrophic waves publication-title: The Hydrodynamics of the Sun contributor: fullname: Shmitt – year: 1985 ident: BIB12 article-title: SPSS-X Advanced Statistics Guide contributor: fullname: Norusis – volume: 110 start-page: 11 year: 1987 ident: BIB15 article-title: The dynamo dilemma publication-title: Solar Phys. contributor: fullname: Parker – volume: 178 start-page: 1863 year: 1972 ident: BIB26 article-title: Dynamo action of global convection in solar convection zone publication-title: Ap. J. contributor: fullname: Yoshimura – volume: 131 start-page: 211 year: 1991 ident: BIB18 article-title: Large-scale flows excited by magnetic fields in the solar convective zone publication-title: Solar Phys. contributor: fullname: Ruzmaikin – volume: 390 start-page: 673 year: 2002 end-page: 680 ident: BIB4 article-title: Parity properties of an advection-dominated solar alpha(2)Omega-dynamo publication-title: Astron.Astrophys. contributor: fullname: Belvedere – volume: 50 start-page: 3 year: 1976 ident: BIB29 article-title: Phase relation between the poloidal and toroidal solar-cycle general magnetic fields and location of the origin of the surface magnetic fields publication-title: Solar Phys. contributor: fullname: Yoshimura – year: 1988 ident: BIB30 article-title: Astrophysics of the Sun contributor: fullname: Zirin – volume: 303 start-page: L29 year: 1995 ident: BIB5 article-title: The solar dynamo with meridional circulation publication-title: Astron. Astrophys. contributor: fullname: Dikpati – volume: V. 12 start-page: 739 year: 2002 end-page: 741 ident: BIB20 article-title: Synthesis of small and large scale dynamos publication-title: Highlights of Astronomy contributor: fullname: Subramanian – volume: 201 start-page: 740 year: 1975 ident: BIB28 article-title: Solar-cycle dynamo wave propagation publication-title: Ap. J. contributor: fullname: Yoshimura – volume: 318 start-page: L55 year: 1997 end-page: L58 ident: BIB23 article-title: The Role of absolute instability in the solar dynamo publication-title: Astron. Astrophys. contributor: fullname: Knobloch – volume: 486 start-page: 484 year: 1997 ident: BIB11 article-title: Solar interface dynamos I. linear, kinematic models in cartesian geometry publication-title: Ap. J. contributor: fullname: Charbonneau – volume: 291 start-page: 49 year: 1969 ident: BIB21 article-title: On the Dynamo Theory of Stellar and Planetary Magnetic Fields. I. AC Dynamos of Solar Type publication-title: Astr. Nach. contributor: fullname: Krause – volume: 394 start-page: 735 year: 2002 end-page: 745 ident: BIB13 article-title: Magnetoconvection and dynamo coefficients. II. Field-direction dependent pumping of magnetic field publication-title: Astron.Astrophys. contributor: fullname: Rudiger – volume: 127 start-page: 221 year: 1991 ident: BIB25 publication-title: Solar Phys. contributor: fullname: Wilson – year: 1981 ident: BIB1 article-title: Cosmic Plasma contributor: fullname: Alfven – volume: 443 start-page: 434 year: 1995 ident: BIB22 article-title: on the spatial distribution of magnetic fields on the solar surface publication-title: Ap. J. contributor: fullname: Cattaneo – volume: 29 start-page: 467 year: 1975 ident: BIB27 article-title: A model of the solar cycle driven by the dynamo action of the global convection in the solar convection zone publication-title: Ap. J. Suppl. Ser. contributor: fullname: Yoshimura – volume: 121 start-page: 491 year: 1955 ident: BIB14 article-title: The Formation of Sunspots from the Solar Toroidal Field publication-title: Ap. J. contributor: fullname: Parker – volume: 110 start-page: 59 year: 1987 ident: BIB24 article-title: Solar rotation and the giant cells publication-title: Solar Phys. contributor: fullname: Wilson – volume: 486 start-page: 1065 year: 1997 ident: BIB9 article-title: On a Babcock-Leighton Solar Dynamo Model with a Deep-seated Generating Layer for the Toroidal Magnetic Field. IV publication-title: Ap. J. contributor: fullname: Durney – volume: 559 start-page: 428 year: 2001 ident: BIB8 article-title: Flux-Transport Dynamos with a-Effect from Global Instability of Tachocline Differential Rotation, A Solution for Magnetic Parity Selection in the Sun publication-title: Ap. J. contributor: fullname: Gilman – volume: 156 start-page: 1 year: 1969 ident: 10.1016/S0273-1177(03)00325-9_BIB10 article-title: A Magneto-Kinematic Model of the Solar Cycle publication-title: Ap. J. doi: 10.1086/149943 contributor: fullname: Leighton – year: 2002 ident: 10.1016/S0273-1177(03)00325-9_BIB3 article-title: Solar and stellar dynamos — latest developments publication-title: Astron. Nachr. doi: 10.1002/1521-3994(200208)323:3/4<411::AID-ASNA411>3.0.CO;2-H contributor: fullname: Brandenburg – volume: 121 start-page: 491 year: 1955 ident: 10.1016/S0273-1177(03)00325-9_BIB14 article-title: The Formation of Sunspots from the Solar Toroidal Field publication-title: Ap. J. doi: 10.1086/146010 contributor: fullname: Parker – volume: 394 start-page: 735 issue: 2 year: 2002 ident: 10.1016/S0273-1177(03)00325-9_BIB13 article-title: Magnetoconvection and dynamo coefficients. II. Field-direction dependent pumping of magnetic field publication-title: Astron.Astrophys. doi: 10.1051/0004-6361:20021224 contributor: fullname: Ossendrijver – volume: 303 start-page: L29 year: 1995 ident: 10.1016/S0273-1177(03)00325-9_BIB5 article-title: The solar dynamo with meridional circulation publication-title: Astron. Astrophys. contributor: fullname: Choudhuri – volume: 443 start-page: 434 year: 1995 ident: 10.1016/S0273-1177(03)00325-9_BIB22 article-title: on the spatial distribution of magnetic fields on the solar surface publication-title: Ap. J. doi: 10.1086/175536 contributor: fullname: Tao – volume: 110 start-page: 59 year: 1987 ident: 10.1016/S0273-1177(03)00325-9_BIB24 article-title: Solar rotation and the giant cells publication-title: Solar Phys. doi: 10.1007/BF00148202 contributor: fullname: Wilson – volume: 291 start-page: 49 year: 1969 ident: 10.1016/S0273-1177(03)00325-9_BIB21 article-title: On the Dynamo Theory of Stellar and Planetary Magnetic Fields. I. AC Dynamos of Solar Type publication-title: Astr. Nach. doi: 10.1002/asna.19692910201 contributor: fullname: Steenbeck – volume: 110 start-page: 11 year: 1987 ident: 10.1016/S0273-1177(03)00325-9_BIB15 article-title: The dynamo dilemma publication-title: Solar Phys. doi: 10.1007/BF00148198 contributor: fullname: Parker – volume: 131 start-page: 211 year: 1991 ident: 10.1016/S0273-1177(03)00325-9_BIB18 article-title: Large-scale flows excited by magnetic fields in the solar convective zone publication-title: Solar Phys. doi: 10.1007/BF00151634 contributor: fullname: Ruzmaikin – volume: 486 start-page: 484 year: 1997 ident: 10.1016/S0273-1177(03)00325-9_BIB11 article-title: Solar interface dynamos I. linear, kinematic models in cartesian geometry publication-title: Ap. J. doi: 10.1086/304484 contributor: fullname: MacGregor – start-page: 223 year: 1984 ident: 10.1016/S0273-1177(03)00325-9_BIB19 article-title: Dynamo action of magnetostrophic waves contributor: fullname: Shmitt – year: 1988 ident: 10.1016/S0273-1177(03)00325-9_BIB30 contributor: fullname: Zirin – year: 1981 ident: 10.1016/S0273-1177(03)00325-9_BIB1 contributor: fullname: Alfven – volume: 133 start-page: 572 year: 1961 ident: 10.1016/S0273-1177(03)00325-9_BIB2 article-title: The topology of the Sun's magnetic field and the 22-year cycle publication-title: Ap. J. doi: 10.1086/147060 contributor: fullname: Babcock – volume: 127 start-page: 221 year: 1991 ident: 10.1016/S0273-1177(03)00325-9_BIB25 publication-title: Solar Phys. doi: 10.1007/BF00146532 contributor: fullname: Wilson – volume: 100 start-page: 125 year: 1985 ident: 10.1016/S0273-1177(03)00325-9_BIB17 article-title: The solar dynamo publication-title: Solar Phys. doi: 10.1007/BF00158425 contributor: fullname: Ruzmaikin – volume: 317 start-page: 610 year: 1997 ident: 10.1016/S0273-1177(03)00325-9_BIB6 article-title: Dynamos with different formulations of a dynamic alpha-effect publication-title: Astron. Astrophys. contributor: fullname: Covas – volume: 178 start-page: 1863 year: 1972 ident: 10.1016/S0273-1177(03)00325-9_BIB26 article-title: Dynamo action of global convection in solar convection zone publication-title: Ap. J. doi: 10.1086/151840 contributor: fullname: Yoshimura – volume: 29 start-page: 467 year: 1975 ident: 10.1016/S0273-1177(03)00325-9_BIB27 article-title: A model of the solar cycle driven by the dynamo action of the global convection in the solar convection zone publication-title: Ap. J. Suppl. Ser. doi: 10.1086/190355 contributor: fullname: Yoshimura – volume: 318 start-page: L55 issue: 2 year: 1997 ident: 10.1016/S0273-1177(03)00325-9_BIB23 article-title: The Role of absolute instability in the solar dynamo publication-title: Astron. Astrophys. contributor: fullname: Tobias – volume: V. 12 start-page: 739 year: 2002 ident: 10.1016/S0273-1177(03)00325-9_BIB20 article-title: Synthesis of small and large scale dynamos contributor: fullname: Subramanian – volume: 390 start-page: 673 year: 2002 ident: 10.1016/S0273-1177(03)00325-9_BIB4 article-title: Parity properties of an advection-dominated solar alpha(2)Omega-dynamo publication-title: Astron.Astrophys. doi: 10.1051/0004-6361:20020590 contributor: fullname: Bonanno – volume: 512 start-page: 417 year: 1999 ident: 10.1016/S0273-1177(03)00325-9_BIB7 article-title: Joint Instability of Latitudinal Differential Rotation and Concentrated Toroidal Fields below the Solar Convection Zone publication-title: Ap. J. doi: 10.1086/306748 contributor: fullname: Dikpati – year: 1985 ident: 10.1016/S0273-1177(03)00325-9_BIB12 contributor: fullname: Norusis – volume: 559 start-page: 428 year: 2001 ident: 10.1016/S0273-1177(03)00325-9_BIB8 article-title: Flux-Transport Dynamos with a-Effect from Global Instability of Tachocline Differential Rotation, A Solution for Magnetic Parity Selection in the Sun publication-title: Ap. J. doi: 10.1086/322410 contributor: fullname: Dikpati – volume: 323 start-page: 432 year: 2002 ident: 10.1016/S0273-1177(03)00325-9_BIB16 article-title: Is the Butterfly diagram due to meridional motions? publication-title: Astr. Nach. doi: 10.1002/1521-3994(200208)323:3/4<432::AID-ASNA432>3.0.CO;2-5 contributor: fullname: Rudiger – volume: 486 start-page: 1065 year: 1997 ident: 10.1016/S0273-1177(03)00325-9_BIB9 article-title: On a Babcock-Leighton Solar Dynamo Model with a Deep-seated Generating Layer for the Toroidal Magnetic Field. IV publication-title: Ap. J. doi: 10.1086/304546 contributor: fullname: Durney – volume: 50 start-page: 3 year: 1976 ident: 10.1016/S0273-1177(03)00325-9_BIB29 article-title: Phase relation between the poloidal and toroidal solar-cycle general magnetic fields and location of the origin of the surface magnetic fields publication-title: Solar Phys. doi: 10.1007/BF00206186 contributor: fullname: Yoshimura – volume: 201 start-page: 740 year: 1975 ident: 10.1016/S0273-1177(03)00325-9_BIB28 article-title: Solar-cycle dynamo wave propagation publication-title: Ap. J. doi: 10.1086/153940 contributor: fullname: Yoshimura |
| SSID | ssj0012770 |
| Score | 1.6849511 |
| Snippet | Using the standard solar w-dynamo equations we formulate appropriate initial and boundary conditions at the moment when the toroidal component is maximum, so... |
| SourceID | proquest crossref elsevier |
| SourceType | Aggregation Database Publisher |
| StartPage | 1175 |
| Title | Nonlinear distribution of the sunspot magnetic field during the solar maximum |
| URI | https://dx.doi.org/10.1016/S0273-1177(03)00325-9 https://search.proquest.com/docview/18040911 https://search.proquest.com/docview/27889251 |
| Volume | 32 |
| hasFullText | 1 |
| inHoldings | 1 |
| isFullTextHit | |
| isPrint | |
| link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwnV3NT9swFH9CoEnjgFjZVBgwHxBiB7dJ7PjjWKGhbhMVElTiFjl2gnpoimgrwYW_fc92ysekatJuieN86OXl936xf-8Z4MSUqV-KklGWWU15bgw1jFtaV6nLtKhLHTK8L0diOOa_bvPbDThf5cJ4WWWL_RHTA1q3Lf3Wmv37yaR_7Sux-ClHdNOEIYv3GewY_tCne88vMo80kzKOs0hGfe_XLJ54hdB4lrDv4SJUr4tPfyF1CD8Xu7DT8kYyiI_2CTaqpgPdwdyPZM-mT-SUhO04UDHvwPabQoMd-HAV2_fgchRrY5gH4nzN3Ha5KzKrCVJBMl_6UucLMjV3jU9vJEHhRmIyY-zh_4Xx-ONkupx-hvHFj5vzIW2XVKCWCb2gBtlWWmaJRlTT1rLc5pnLuPPiEWGEcYY7K4V0mmuFO0pYm1SiTGqMdpJx9gU2m1lTdYEkrCqFqoTMVM05zxUyISsdMkhWCqeTfeitDFncx8oZxaukDC3f1hlnRbB8ofdBrcxdvHOBAtH9X6d-W72eAj8PP-dhmmq2nBepQpRCQF_fI5NKaWR5B_9_-6_wMWj8gvTsEDYXD8vqCLnKojwOzngMW4Ofv4ejP8Wk5FY |
| link.rule.ids | 315,783,787,4509,24128,27936,27937,45597,45691 |
| linkProvider | Elsevier |
| linkToHtml | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwnV3PT9swFH4CJgQ7TKMwwX7hA5rgYJrEjn8cERrqNlpNGkjcLMdOph6aVrSV4MLfvmc7HRsSmrRb4jhO9PLy-bP93meAI1vlYStKRlnhNOWltdQy7mhT577Qoql0zPAejsTgmn-9KW_W4HyVCxPCKjvsT5ge0bor6XfW7M_G4_6PoMQSlhzRTTOGLH4dXvDAj9GpTx9-x3nkhZRpokUyGqo_pvGkJmLhccZOYitUP9dBPYHq2P9cvIZXHXEkZ-nddmCtbnuwfzYPU9nTyT35ROJxmqmY9-DlH0qDPdj8nsp3YThK4hj2lvggmtvtd0WmDUEuSObLoHW-IBP7sw35jSSGuJGUzZhqhMEwXr8bT5aTPbi--Hx1PqDdngrUMaEX1CLdyqsi0whr2jlWurLwBfchekRYYb3l3kkhveZa4YkSzmW1qLIGuzvJOHsDG-20rfeBZKyuhKqFLFTDOS8VUiEnPVJIVgmvswM4XRnSzJJ0hnmMKUPLd0LjzETLG30AamVu85cPGIT3f916uPo8Bv-PsOhh23q6nJtcIUwhoj9fo5BKaaR5b___8YewNbgaXprLL6Nv72A7BvzFOLT3sLG4XdYfkLgsqo_RMX8BMMHl7w |
| openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Nonlinear+distribution+of+the+sunspot+magnetic+field+during+the+solar+maximum&rft.jtitle=Advances+in+space+research&rft.au=Rosa%2C+R+R&rft.au=Gonzalez-Machado%2C+E.A.M.&rft.au=Boechat-Roberty%2C+H+M&rft.au=Vijaykumar%2C+N+L&rft.date=2003-09-01&rft.issn=0273-1177&rft.volume=32&rft.issue=6&rft.spage=1175&rft.epage=1180&rft_id=info:doi/10.1016%2FS0273-1177%2803%2900325-9&rft.externalDBID=NO_FULL_TEXT |
| thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0273-1177&client=summon |
| thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0273-1177&client=summon |
| thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0273-1177&client=summon |