Are magnetic dips necessary for prominence formation?

被引：171
作者：
Karpen, JT [1 ]
Antiochos, SK
Hohensee, M
Klimchuk, JA
MacNeice, PJ
机构：
[1] USN, Res Lab, EO Hulburt Ctr Space Res, Washington, DC 20375 USA
[2] Drexel Univ, Dept Phys & Atmospher Sci, Philadelphia, PA 19104 USA
来源：
ASTROPHYSICAL JOURNAL | 2001年 / 553卷 / 01期
基金：
美国国家航空航天局;
关键词：
Sun : chromosphere; Sun : corona; Sun : prominences;
D O I：
10.1086/320497
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The short answer: No.
引用
收藏
页码：L85 / L88
页数：4
相关论文
共 29 条
  • [1] THE MAGNETIC-FIELD OF SOLAR PROMINENCES
    ANTIOCHOS, SK
    DAHLBURG, RB
    KLIMCHUK, JA
    [J]. ASTROPHYSICAL JOURNAL, 1994, 420 (01) : L41 - L44
  • [2] A MODEL FOR THE FORMATION OF SOLAR PROMINENCES
    ANTIOCHOS, SK
    KLIMCHUK, JA
    [J]. ASTROPHYSICAL JOURNAL, 1991, 378 (01) : 372 - 377
  • [3] The thermal nonequilibrium of prominences
    Antiochos, SK
    MacNeice, PJ
    Spicer, DS
    [J]. ASTROPHYSICAL JOURNAL, 2000, 536 (01) : 494 - 499
  • [4] The dynamic formation of prominence condensations
    Antiochos, SK
    MacNeice, PJ
    Spicer, DS
    Klimchuk, JA
    [J]. ASTROPHYSICAL JOURNAL, 1999, 512 (02) : 985 - 991
  • [5] Anzer U, 2000, ASTRON ASTROPHYS, V358, pL75
  • [6] IRON IONIZATION AND RECOMBINATION RATES AND IONIZATION EQUILIBRIUM
    ARNAUD, M
    RAYMOND, J
    [J]. ASTROPHYSICAL JOURNAL, 1992, 398 (01) : 394 - 406
  • [7] Evidence for nonuniform heating of coronal loops inferred from multithread modeling of TRACE data
    Aschwanden, MJ
    Nightingale, RW
    Alexander, D
    [J]. ASTROPHYSICAL JOURNAL, 2000, 541 (02) : 1059 - 1077
  • [8] Modeling of coronal EUV loops observed with TRACE.: I.: Hydrostatic solutions with nonuniform heating
    Aschwanden, MJ
    Schrijver, CJ
    Alexander, D
    [J]. ASTROPHYSICAL JOURNAL, 2001, 550 (02) : 1036 - 1050
  • [9] Aulanier G, 1998, ASTRON ASTROPHYS, V329, P1125
  • [10] Prominence formation by localized heating
    Dahlburg, RB
    Antiochos, SK
    Klimchuk, JA
    [J]. ASTROPHYSICAL JOURNAL, 1998, 495 (01) : 485 - 490
123