RECOMBINATION COEFFICIENT AND CORONAL CONTRIBUTION TO E-LAYER IONIZATION FROM MAGNETIC OBSERVATIONS OF A SOLAR ECLIPSE

被引：17
|
作者：
BOMKE, HA
BLAKE, HA
HARRIS, AK
HULSE, WH
SHEPPARD, DJ
机构：
来源：
JOURNAL OF GEOPHYSICAL RESEARCH | 1967年 / 72卷 / 23期
关键词：
D O I：
10.1029/JZ072i023p05913
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
引用
收藏
页码：5913 / +
页数：1
相关论文
共 48 条
  • [31] Study of the Green Coronal Line with Altitude from Out-of-Eclipse Observations during Solar Cycle 24
    S. A. Guseva
    A. D. Shramko
    Cosmic Research, 2023, 61 : 133 - 141
  • [32] Identifying the Coronal Source Regions of Solar Wind Streams from Total Solar Eclipse Observations and in situ Measurements Extending over a Solar Cycle
    Habbal, Shadia R.
    Druckmuller, Miloslav
    Alzate, Nathalia
    Ding, Adalbert
    Johnson, Judd
    Starha, Pavel
    Hoderova, Jana
    Boe, Benjamin
    Constantinou, Sage
    Arndt, Martina
    ASTROPHYSICAL JOURNAL LETTERS, 2021, 911 (01)
  • [33] From solar and stellar flares to coronal heating: Theory and observations of how magnetic reconnection regulates coronal conditions
    Cassak, P. A.
    Mullan, D. J.
    Shay, M. A.
    ASTROPHYSICAL JOURNAL LETTERS, 2008, 676 (01) : L69 - L72
  • [34] AN ESTIMATE OF THE CORONAL MAGNETIC FIELD NEAR A SOLAR CORONAL MASS EJECTION FROM LOW-FREQUENCY RADIO OBSERVATIONS
    Hariharan, K.
    Ramesh, R.
    Kishore, P.
    Kathiravan, C.
    Gopalswamy, N.
    ASTROPHYSICAL JOURNAL, 2014, 795 (01):
  • [35] THERMODYNAMICS OF THE SOLAR CORONA AND EVOLUTION OF THE SOLAR MAGNETIC FIELD AS INFERRED FROM THE TOTAL SOLAR ECLIPSE OBSERVATIONS OF 2010 JULY 11
    Habbal, Shadia Rifai
    Druckmueller, Miloslav
    Morgan, Huw
    Ding, Adalbert
    Johnson, Judd
    Druckmuellerova, Hana
    Daw, Adrian
    Arndt, Martina B.
    Dietzel, Martin
    Saken, Jon
    ASTROPHYSICAL JOURNAL, 2011, 734 (02):
  • [36] On the possibility of determining the coronal magnetic field from solar type III radio burst observations
    Ledenev, VG
    Messerotti, M
    SOLAR PHYSICS, 1999, 185 (01) : 193 - 204
  • [37] GE))THE EFFECT OF SOFT X-RAYS FROM THE SOLAR CORONA ON THE FORMATION OF THE NORMAL IONOSPHERIC E-LAYER
    ELWERT, G
    JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1953, 4 (1-2): : 68 - 77
  • [38] On the possibility of determining the coronal magnetic field from solar type III radio burst observations
    V.G. Ledenev
    M. Messerotti
    Solar Physics, 1999, 185 : 193 - 204
  • [39] Dynamics of coronal magnetic fields inferred from multi-frequency radio observations of a solar flare
    Correia, E
    Raulin, JP
    Trottet, G
    Kaufmann, P
    MULTI-WAVELENGTH OBSERVATIONS OF CORONAL STRUCTURE AND DYNAMICS, 2002, 13 : 229 - 231
  • [40] SOME NEWLY DISCOVERED CORONAL EMISSION-LINES FROM HIGH-ALTITUDE INFRARED OBSERVATIONS OF 7 MARCH, 1970, SOLAR ECLIPSE
    OLSEN, KH
    ANDERSON, CR
    STEWART, JN
    SOLAR PHYSICS, 1971, 21 (02) : 360 - +
12345